

<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://strike.scec.org/scecwiki/api.php?action=feedcontributions&amp;feedformat=atom&amp;user=Goulet</id>
	<title>SCECpedia - User contributions [en]</title>
	<link rel="self" type="application/atom+xml" href="https://strike.scec.org/scecwiki/api.php?action=feedcontributions&amp;feedformat=atom&amp;user=Goulet"/>
	<link rel="alternate" type="text/html" href="https://strike.scec.org/scecpedia/Special:Contributions/Goulet"/>
	<updated>2026-04-26T08:15:58Z</updated>
	<subtitle>User contributions</subtitle>
	<generator>MediaWiki 1.34.2</generator>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24950</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24950"/>
		<updated>2020-09-10T18:07:29Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Observational Data */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Events Considered ==&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38443183/moment-tensor USGS Event page for M6.4 (RIDG19A)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38450263/moment-tensor USGS Event page for M5.4 (RIDG19B)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38457511/moment-tensor USGS Event page for M7.1 (RIDG19C)]&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_Ridg19_Flatfile_RotD50_050_EventParameters.xlsx Source information from NGA-NHR3 preliminary release]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-NHR3-processed data available as of 2020-06-09]&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/GEFileVs30map_FaultTraces_Ridgecrest_All3NonRepeat_name.kml Google Earth map of Vs30 at recording stations (triangles=measured and circles=inferred)]&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;br /&gt;
* For the validation, Christine selected all the stations within a closest distance (Rrup) of 125 km of all three events. This yielded ~ 50 stations, most of which have recordings for all three events.&lt;br /&gt;
&lt;br /&gt;
== SRC Files ==&lt;br /&gt;
&lt;br /&gt;
=== M5.4 ===&lt;br /&gt;
&lt;br /&gt;
 MAGNITUDE = 5.36&lt;br /&gt;
 LAT_TOP_CENTER = 35.757359&lt;br /&gt;
 LON_TOP_CENTER = -117.566269&lt;br /&gt;
 DEPTH_TO_TOP = 6.0&lt;br /&gt;
 STRIKE = 313&lt;br /&gt;
 DIP = 81&lt;br /&gt;
 RAKE = -165&lt;br /&gt;
 FAULT_LENGTH = 3.0&lt;br /&gt;
 DLEN = 0.1&lt;br /&gt;
 FAULT_WIDTH = 3.0&lt;br /&gt;
 DWID = 0.1&lt;br /&gt;
 HYPO_ALONG_STK = 0.0&lt;br /&gt;
 HYPO_DOWN_DIP = 1.5&lt;br /&gt;
 SEED = ***needs_to_be_specified_and_different_than_other_segments_and_hypos***&lt;br /&gt;
 MAX_FAULT_LENGTH = 3&lt;br /&gt;
 RUPTURE_DELAY = 0.00&lt;br /&gt;
 MOMENT_FRACTION = 1&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24655</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24655"/>
		<updated>2020-06-25T00:06:06Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Station Selection */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Events Considered ==&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38443183/moment-tensor USGS Event page for M6.4 (RIDG19A)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38450263/moment-tensor USGS Event page for M5.4 (RIDG19B)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38457511/moment-tensor USGS Event page for M7.1 (RIDG19C)]&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_Ridg19_Flatfile_RotD50_050_EventParameters.xlsx Source information from NGA-NHR3 preliminary release]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-NHR3-processed data available as of 2020-06-09]&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;br /&gt;
* For the validation, Christine selected all the stations within a closest distance (Rrup) of 125 km of all three events. This yielded ~ 50 stations, most of which have recordings for all three events.&lt;br /&gt;
&lt;br /&gt;
== SRC Files ==&lt;br /&gt;
&lt;br /&gt;
=== M5.4 ===&lt;br /&gt;
&lt;br /&gt;
 MAGNITUDE = 5.36&lt;br /&gt;
 LAT_TOP_CENTER = 35.757359&lt;br /&gt;
 LON_TOP_CENTER = -117.566269&lt;br /&gt;
 DEPTH_TO_TOP = 6.0&lt;br /&gt;
 STRIKE = 313&lt;br /&gt;
 DIP = 81&lt;br /&gt;
 RAKE = -165&lt;br /&gt;
 FAULT_LENGTH = 3.0&lt;br /&gt;
 DLEN = 0.1&lt;br /&gt;
 FAULT_WIDTH = 3.0&lt;br /&gt;
 DWID = 0.1&lt;br /&gt;
 HYPO_ALONG_STK = 0.0&lt;br /&gt;
 HYPO_DOWN_DIP = 1.5&lt;br /&gt;
 SEED = ***needs_to_be_specified_and_different_than_other_segments_and_hypos***&lt;br /&gt;
 MAX_FAULT_LENGTH = 3&lt;br /&gt;
 RUPTURE_DELAY = 0.00&lt;br /&gt;
 MOMENT_FRACTION = 1&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24654</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24654"/>
		<updated>2020-06-24T22:54:12Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_La_Habra_Verification High-F 2020 continuation of verification]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_La_Habra_Verification&amp;diff=24653</id>
		<title>HighF La Habra Verification</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_La_Habra_Verification&amp;diff=24653"/>
		<updated>2020-06-24T22:52:23Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2020 verification runs for four groups: Olsen et al. (AWP), Graves (RWG) and Taborda, Restrepo et al. (Hercules), Breuer (Edge). Verification of 5 Hz time series (4Hz PSA, multiple bands verification) using La Habra stations.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Path forward on VERIFICATION paper ==&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use medium domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the medium domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
===== BBP Station List =====&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob &lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. &lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
===== Source model =====&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. [http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Combined results from all groups here!]&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_2018 High-F 2018-2019 notes]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_La_Habra_Verification&amp;diff=24652</id>
		<title>HighF La Habra Verification</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_La_Habra_Verification&amp;diff=24652"/>
		<updated>2020-06-24T22:51:10Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2020 verification runs for four groups: Olsen et al. (AWP), Graves (RWG) and Taborda, Restrepo et al. (Hercules), Breuer (Edge). Verification of 5 Hz time series (4Hz PSA, multiple bands verification) using La Habra stations.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Path forward on VERIFICATION paper ==&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use medium domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the medium domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
===== BBP Station List =====&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob &lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. &lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
===== Source model =====&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. [http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Combined results from all groups here!]&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_La_Habra_Verification&amp;diff=24651</id>
		<title>HighF La Habra Verification</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_La_Habra_Verification&amp;diff=24651"/>
		<updated>2020-06-24T22:50:08Z</updated>

		<summary type="html">&lt;p&gt;Goulet: Created page with &amp;quot;This page documents the High-F activities and decisions for the 2020 verification runs for four groups: Olsen et al. (AWP), Graves (RWG) and Taborda, Restrepo et al. (Hercules...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2020 verification runs for four groups: Olsen et al. (AWP), Graves (RWG) and Taborda, Restrepo et al. (Hercules), Breuer (Edge). Verification of 5 Hz time series (4Hz PSA, multiple bands verification) using La Habra stations.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Path forward on VERIFICATION paper ==&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use medium domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the medium domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
==== BBP Station List ====&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob &lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. &lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
==== Source model ====&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. [http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Combined results from all groups here!]&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24650</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24650"/>
		<updated>2020-06-24T22:44:27Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use medium domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the medium domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
==== BBP Station List ====&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob &lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. &lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
==== Source model ====&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. [http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Combined results from all groups here!]&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24649</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24649"/>
		<updated>2020-06-24T22:42:03Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== BBP Station List ====&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. Please see below the BBP station list for the 15 stations listed above:&lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. [http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Combined results from all groups here!]&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24648</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24648"/>
		<updated>2020-06-24T22:39:52Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== BBP Station List ====&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. Please see below the BBP station list for the 15 stations listed above:&lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. [http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Combined results from all groups here!]&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24647</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24647"/>
		<updated>2020-06-24T22:39:14Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== BBP Station List ====&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. Please see below the BBP station list for the 15 stations listed above:&lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
*Step 1 was completed on June 17 during our call, at which time we moved to Step 2 below. ([http://hypocenter.usc.edu/bbp/highf/2020-06-18/combined-06-17/ Results here!])&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24646</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24646"/>
		<updated>2020-06-24T22:36:07Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 2: verification with the selected source, using the large domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== USGS Earthquake Information ==&lt;br /&gt;
*[[La Habra Earthquake]]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
*[[La_Habra_Observational_Data]]&lt;br /&gt;
*[[Selection_of_La_Habra_Ground_Motion_Observations]]&lt;br /&gt;
&lt;br /&gt;
== Region Definitions ==&lt;br /&gt;
*[[La_Habra_Simulation_Region]]&lt;br /&gt;
*[[La Habra Simulations on Titan]]&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
*Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
*Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
*Proposed medium domain:&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
The four corners of medium La Habra Simulation domain are:&lt;br /&gt;
 c1= -118.387131  33.887287&lt;br /&gt;
 c2= -117.970993  34.301479&lt;br /&gt;
 c3= -117.472496  33.955025&lt;br /&gt;
 c4= -117.889359  33.542511&lt;br /&gt;
And the model dimensions are:&lt;br /&gt;
 xlen=    60.0000 km&lt;br /&gt;
 ylen=    60.0000 km&lt;br /&gt;
 zlen=    25.0000 km&lt;br /&gt;
&lt;br /&gt;
Note that this is not a UTM projection. It is transverse Mercator with spherical reference and corresponds very closely to the proj4 projection: &lt;br /&gt;
+proj=tmerc +lat_0=%f +lon_0=%f +ellps=sphere +a=6378139.0 +b=6378139.0 +units=m +no_defs&lt;br /&gt;
&lt;br /&gt;
where lat_0, lon_0 are the domain center coordinates, which in this case are: lon= -117.930000 lat=  33.922000&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The regional seismic velocity model used by all modelers is:  CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** We retrieved the Vs30 values using UCVM v19.4 for CVM-S4.26.M01 (cvmsi), for CVM-S4.26 (to show impact of adding .M01 GTL), for CVM-S4 (to check if Vs30 matches .M01 exactly), and from the Wills 2015 Vs30 model embedded in UCVM. &lt;br /&gt;
* For the Vs30_query against the models uses a slowness algorithm, and a 1 meter spacing. &lt;br /&gt;
* The Wills 2015 Vs30 values are based a processing sequence that includes converting a GIS shape file into a rasterized Vs30 grid of values produced by Kevin Milner. Kevin provided a file raster_0.00025.flt, which is rasterized with 0.00025 degree spacing (~25 meters). This file is then used to generate an etree which is used to stored the rasterized data. When query points are given between grid points, then ucvm implements interplolation of Vs30 values between associated grid points. More&lt;br /&gt;
* More details on the Willis Map integration here: [[Wills Map]].&lt;br /&gt;
* Descriptions of UCVM Vs30 Slowness algorithm here: [[UCVM_Vs30]].&lt;br /&gt;
* Description of CyberShake Vs30 Slowness algorithm here: [[CyberShake_Code_Base#Stochastic%20codes]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+UCVM Vs30 Values&lt;br /&gt;
|-&lt;br /&gt;
|Station Id&lt;br /&gt;
|Lat - NGA-West2&lt;br /&gt;
|Lon - NGA-West2&lt;br /&gt;
|Vs30 - NGA-West2&lt;br /&gt;
|Vs30 - Wills 2015 (UCVM v19.4)&lt;br /&gt;
|Vs30 - Slowness Method (1m res) CVM-S4.26.M01 (cvmsi) (UCVM v19.4)&lt;br /&gt;
|-&lt;br /&gt;
| CE_13066&lt;br /&gt;
| -117.9568&lt;br /&gt;
| 33.8401&lt;br /&gt;
| 288.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 284.461&lt;br /&gt;
|-&lt;br /&gt;
| CE_13849&lt;br /&gt;
| -117.8180&lt;br /&gt;
| 33.8535&lt;br /&gt;
| 385.00&lt;br /&gt;
| 351.900&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_13878&lt;br /&gt;
| -117.8870&lt;br /&gt;
| 33.8891&lt;br /&gt;
| 398.00&lt;br /&gt;
| 313.585&lt;br /&gt;
| 344.043&lt;br /&gt;
|-&lt;br /&gt;
| CE_13879&lt;br /&gt;
| -117.9591&lt;br /&gt;
| 33.8663&lt;br /&gt;
| 299.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_13880&lt;br /&gt;
| -117.9311&lt;br /&gt;
| 33.9086&lt;br /&gt;
| 324.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.812&lt;br /&gt;
|-&lt;br /&gt;
| CE_13881&lt;br /&gt;
| -117.9557&lt;br /&gt;
| 33.9315&lt;br /&gt;
| 353.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 349.317&lt;br /&gt;
|-&lt;br /&gt;
| CE_13882&lt;br /&gt;
| -117.8034&lt;br /&gt;
| 33.9274&lt;br /&gt;
| 412.00&lt;br /&gt;
| 385.100&lt;br /&gt;
| 367.423&lt;br /&gt;
|-&lt;br /&gt;
| CE_13883&lt;br /&gt;
| -117.8578&lt;br /&gt;
| 33.8534&lt;br /&gt;
| 300.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 329.762&lt;br /&gt;
|-&lt;br /&gt;
| CE_14026&lt;br /&gt;
| -118.0469&lt;br /&gt;
| 33.8892&lt;br /&gt;
| 281.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 287.845&lt;br /&gt;
|-&lt;br /&gt;
| CE_14027&lt;br /&gt;
| -118.0576&lt;br /&gt;
| 33.9283&lt;br /&gt;
| 342.00&lt;br /&gt;
| 386.600&lt;br /&gt;
| 354.637&lt;br /&gt;
|-&lt;br /&gt;
| CE_23938&lt;br /&gt;
| -117.8657&lt;br /&gt;
| 34.0209&lt;br /&gt;
| 402.00&lt;br /&gt;
| 418.980&lt;br /&gt;
| 370.670&lt;br /&gt;
|-&lt;br /&gt;
| CI_BRE&lt;br /&gt;
| -117.9812&lt;br /&gt;
| 33.8078&lt;br /&gt;
| 238.00&lt;br /&gt;
| 228.200&lt;br /&gt;
| 285.871&lt;br /&gt;
|-&lt;br /&gt;
| CI_FUL&lt;br /&gt;
| -117.9225&lt;br /&gt;
| 33.8717&lt;br /&gt;
| 309.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 362.574&lt;br /&gt;
|-&lt;br /&gt;
| CI_OLI&lt;br /&gt;
| -117.9237&lt;br /&gt;
| 33.9454&lt;br /&gt;
| 328.00&lt;br /&gt;
| 385.433&lt;br /&gt;
| 331.459&lt;br /&gt;
|-&lt;br /&gt;
| CI_WLT&lt;br /&gt;
| -117.9508&lt;br /&gt;
| 34.0095&lt;br /&gt;
| 265.00&lt;br /&gt;
| 293.500&lt;br /&gt;
| 309.646&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== BBP Station List ====&lt;br /&gt;
&lt;br /&gt;
The BBP station list was updated to include station latitude and longitude coordinates up to 4 decimal places. It includes the Vs30 from the NGA-West2 flat file, updated on May 12th, 2020. Please see below the BBP station list for the 15 stations listed above:&lt;br /&gt;
&lt;br /&gt;
 -117.9568 33.8401  CE_13066  288.00  0.1250  4.0000&lt;br /&gt;
 -117.8180 33.8535  CE_13849  385.00  0.1250  4.0000&lt;br /&gt;
 -117.8870 33.8891  CE_13878  398.00  0.1250  4.0000&lt;br /&gt;
 -117.9591 33.8663  CE_13879  299.00  0.1250  4.0000&lt;br /&gt;
 -117.9311 33.9086  CE_13880  324.00  0.1250  4.0000&lt;br /&gt;
 -117.9557 33.9315  CE_13881  353.00  0.1250  4.0000&lt;br /&gt;
 -117.8034 33.9274  CE_13882  412.00  0.1250  4.0000&lt;br /&gt;
 -117.8578 33.8534  CE_13883  300.00  0.1250  4.0000&lt;br /&gt;
 -118.0469 33.8892  CE_14026  281.00  0.1250  4.0000&lt;br /&gt;
 -118.0576 33.9283  CE_14027  342.00  0.1250  4.0000&lt;br /&gt;
 -117.8657 34.0209  CE_23938  402.00  0.1250  4.0000&lt;br /&gt;
 -117.9812 33.8078  CI_BRE  238.00  0.1250  4.0000&lt;br /&gt;
 -117.9225 33.8717  CI_FUL  309.00  0.1250  4.0000&lt;br /&gt;
 -117.9237 33.9454  CI_OLI  328.00  0.1250  4.0000&lt;br /&gt;
 -117.9508 34.0095  CI_WLT  265.00  0.1250  4.0000&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** We agreed to keep the same rotation as for the small domain (39.9 degrees)&lt;br /&gt;
** need to review the station list and post it HERE&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24641</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24641"/>
		<updated>2020-06-18T22:54:28Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Events Considered ==&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38443183/moment-tensor USGS Event page for M6.4 (RIDG19A)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38450263/moment-tensor USGS Event page for M5.4 (RIDG19B)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38457511/moment-tensor USGS Event page for M7.1 (RIDG19C)]&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_Ridg19_Flatfile_RotD50_050_EventParameters.xlsx Source information from NGA-NHR3 preliminary release]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-NHR3-processed data available as of 2020-06-09]&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;br /&gt;
* For the validation, we select the 50 stations closest to the hypocenter of the M5.4 event&lt;br /&gt;
&lt;br /&gt;
== SRC Files ==&lt;br /&gt;
&lt;br /&gt;
=== M5.4 ===&lt;br /&gt;
&lt;br /&gt;
 MAGNITUDE = 5.36&lt;br /&gt;
 LAT_TOP_CENTER = 35.757359&lt;br /&gt;
 LON_TOP_CENTER = -117.566269&lt;br /&gt;
 DEPTH_TO_TOP = 6.0&lt;br /&gt;
 STRIKE = 313&lt;br /&gt;
 DIP = 81&lt;br /&gt;
 RAKE = -165&lt;br /&gt;
 FAULT_LENGTH = 3.0&lt;br /&gt;
 DLEN = 0.1&lt;br /&gt;
 FAULT_WIDTH = 3.0&lt;br /&gt;
 DWID = 0.1&lt;br /&gt;
 HYPO_ALONG_STK = 0.0&lt;br /&gt;
 HYPO_DOWN_DIP = 1.5&lt;br /&gt;
 SEED = ***needs_to_be_specified_and_different_than_other_segments_and_hypos***&lt;br /&gt;
 MAX_FAULT_LENGTH = 3&lt;br /&gt;
 RUPTURE_DELAY = 0.00&lt;br /&gt;
 MOMENT_FRACTION = 1&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24640</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24640"/>
		<updated>2020-06-18T22:51:25Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Events Considered */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Events Considered ==&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38443183/moment-tensor USGS Event page for M6.4 (RIDG19A)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38450263/moment-tensor USGS Event page for M5.4 (RIDG19B)]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38457511/moment-tensor USGS Event page for M7.1 (RIDG19C)]&lt;br /&gt;
&lt;br /&gt;
Source information from NHR3 preliminary release&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;br /&gt;
* For the validation, we select the 50 stations closest to the hypocenter of the M5.4 event&lt;br /&gt;
&lt;br /&gt;
== SRC Files ==&lt;br /&gt;
&lt;br /&gt;
=== M5.4 ===&lt;br /&gt;
&lt;br /&gt;
 MAGNITUDE = 5.36&lt;br /&gt;
 LAT_TOP_CENTER = 35.757359&lt;br /&gt;
 LON_TOP_CENTER = -117.566269&lt;br /&gt;
 DEPTH_TO_TOP = 6.0&lt;br /&gt;
 STRIKE = 313&lt;br /&gt;
 DIP = 81&lt;br /&gt;
 RAKE = -165&lt;br /&gt;
 FAULT_LENGTH = 3.0&lt;br /&gt;
 DLEN = 0.1&lt;br /&gt;
 FAULT_WIDTH = 3.0&lt;br /&gt;
 DWID = 0.1&lt;br /&gt;
 HYPO_ALONG_STK = 0.0&lt;br /&gt;
 HYPO_DOWN_DIP = 1.5&lt;br /&gt;
 SEED = ***needs_to_be_specified_and_different_than_other_segments_and_hypos***&lt;br /&gt;
 MAX_FAULT_LENGTH = 3&lt;br /&gt;
 RUPTURE_DELAY = 0.00&lt;br /&gt;
 MOMENT_FRACTION = 1&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24624</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24624"/>
		<updated>2020-06-10T22:03:54Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Events Considered ==&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38450263/moment-tensor USGS Event page for M5.4]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38443183/moment-tensor USGS Event page for M6.4]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38457511/moment-tensor USGS Event page for M7.1]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;br /&gt;
* For the validation, we select the 50 stations closest to the hypocenter of the M5.4 event&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24623</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24623"/>
		<updated>2020-06-10T22:02:28Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Events and information ==&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38450263/moment-tensor USGS Event page for M5.4]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38443183/moment-tensor USGS Event page for M6.4]&lt;br /&gt;
* [https://earthquake.usgs.gov/earthquakes/eventpage/ci38457511/moment-tensor USGS Event page for M7.1]&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24621</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24621"/>
		<updated>2020-06-09T19:03:28Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence.&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Station Selection ==&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24620</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24620"/>
		<updated>2020-06-09T18:07:16Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Observational Data */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecrestSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24619</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24619"/>
		<updated>2020-06-09T18:06:57Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/BBP_RidgecretSequence/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24618</id>
		<title>BBP Group Ridgecrest Sequence Simulations</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=BBP_Group_Ridgecrest_Sequence_Simulations&amp;diff=24618"/>
		<updated>2020-06-09T18:06:03Z</updated>

		<summary type="html">&lt;p&gt;Goulet: Created page with &amp;quot;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence  == Observational Data == * [http://hypocenter.usc.edu/research/Goulet/2019RidgEqS...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the BBP Group activities to simulate events from the Ridgecrest Sequence&lt;br /&gt;
&lt;br /&gt;
== Observational Data ==&lt;br /&gt;
* [http://hypocenter.usc.edu/research/Goulet/2019RidgEqSeq_NGA_Datasets_20200609.kmz Google Earth map of NGA-processed data available as of 2020-06-09]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24218</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24218"/>
		<updated>2020-04-14T00:45:57Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24217</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24217"/>
		<updated>2020-04-14T00:44:35Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RWG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24216</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24216"/>
		<updated>2020-04-14T00:43:53Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain, with Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)) and constraints, [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24215</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24215"/>
		<updated>2020-04-14T00:38:04Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Simulation results */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24214</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24214"/>
		<updated>2020-04-14T00:37:40Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on 15 near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24213</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24213"/>
		<updated>2020-04-14T00:37:22Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here, file to include Vs30 values listed above: from NGA-West2 or Wills et al. 2015 and from the cvm)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24212</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24212"/>
		<updated>2020-04-14T00:36:11Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Step 1: selection and verification of source model using the small domain */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models. This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24211</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24211"/>
		<updated>2020-04-14T00:35:01Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Vs30 at recording stations */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil to retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24210</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24210"/>
		<updated>2020-04-14T00:33:50Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 at recording stations ====&lt;br /&gt;
* For interpretation of recorded data, use in order of preference &lt;br /&gt;
** values listed as &amp;quot;Vs30 (m/s) selected for analysis&amp;quot; in the NGA-West2 database flatfile&lt;br /&gt;
** if stations are not included in the NGA-West2 database, we will use the values from Will et al. 2015 as retrieved from UCVM (with interpolation) &lt;br /&gt;
* For interpretation of simulation data&lt;br /&gt;
** Phil will retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation).&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24209</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24209"/>
		<updated>2020-04-14T00:28:50Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
=== Misc definitions ===&lt;br /&gt;
==== Domains ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
==== Vs30 ====&lt;br /&gt;
* We will use those listed as &amp;quot;Used for analysis&amp;quot; in the NGA-West2 database for interpretation purposes of the data; if stations are not included in the NGA-West2 database, we will use the values retrieved from Will et al. 2015 as retrieved from UCVM (with interpolation). &lt;br /&gt;
* Phil will retrieve the Vs30 values computed from the UCVM algorithm for cmvsi (includes interpolation), for interpretation purposes of the simulations.&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24208</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24208"/>
		<updated>2020-04-14T00:22:38Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
==== Domain definitions ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification with the selected source, using the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24207</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24207"/>
		<updated>2020-04-14T00:21:58Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
==== Domain definitions ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification among modelers for the selected source, applied to the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
=== Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24206</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24206"/>
		<updated>2020-04-14T00:21:36Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
==== Domain definitions ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification among modelers for the selected source, applied to the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
 === Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24205</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24205"/>
		<updated>2020-04-14T00:21:19Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
==== Domain definitions ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification among modelers for the selected source, applied to the large domain === &lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
&lt;br /&gt;
 === Step 3: write paper, publish  ===&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24204</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24204"/>
		<updated>2020-04-14T00:20:28Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification)&lt;br /&gt;
&lt;br /&gt;
==== Domain definitions ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
=== Step 2: verification among modelers for the selected source, applied to the large domain&lt;br /&gt;
* Then all modelers rerun large region &lt;br /&gt;
** need to confer on rotations before that step&lt;br /&gt;
** need to review the station list&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** tsprocess time series/FAS/PSA combo plots&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24203</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24203"/>
		<updated>2020-04-14T00:18:16Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
==== Domain definitions ====&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24202</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24202"/>
		<updated>2020-04-14T00:17:51Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020 updates from weekly calls: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
Domain definitions&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Step 1: selection and verification of source model using the small domain === 	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24201</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24201"/>
		<updated>2020-04-14T00:17:13Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020-03-16 call summary: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020 updates from weekly calls: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Step 1: selection and verification of source model using the small domain	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24200</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24200"/>
		<updated>2020-04-14T00:16:07Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Step 1: selection and verification of source model	&lt;br /&gt;
* Use small domain&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
* Use RWG best source:&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24199</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24199"/>
		<updated>2020-04-14T00:13:48Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints  apply the rules described here].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Step 1: selection and verification of source model	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24198</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24198"/>
		<updated>2020-04-14T00:13:06Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described here.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Step 1: selection and verification of source model	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24197</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24197"/>
		<updated>2020-04-14T00:11:59Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020-03-16 call summary: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
&lt;br /&gt;
Step 1: selection and verification of source model	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24196</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24196"/>
		<updated>2020-04-14T00:11:39Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020-03-16 call summary: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
Step 1: selection and verification of source model	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model or different constraints.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24195</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24195"/>
		<updated>2020-04-14T00:10:14Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020-03-16 call summary: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):&lt;br /&gt;
Step 1: selection and verification of source model	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]). This is a first-order test for the purpose of the verification paper only, modelers can chose another source for the validation paper later, if, for example, they use another velocity model.&lt;br /&gt;
* We agreed that all the modelers will use a version of the small domain that is rotated by 39.9 degrees, so as to remove a source of difference we can control. We observed different results due to rotation of the domain in CyberShake simulations a few months ago, for which we could not account for by considering the model edges and boundary effects. There seems to be some anisotropy in the model that may be due to the staggered grid.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24194</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24194"/>
		<updated>2020-04-14T00:04:13Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020-03-16 call summary: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models ([https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1 here]) &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24193</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24193"/>
		<updated>2020-04-14T00:02:53Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi)), [https://scec.usc.edu/scecpedia/HighF_2018#Mesh_generation_rules_and_parameter_constraints as described here] &lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models[https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1]) &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24192</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24192"/>
		<updated>2020-04-14T00:02:05Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi))&lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models[https://scec.usc.edu/scecpedia/HighF_2018#Site_Selection see 2020 updates, Step 1]) &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24191</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24191"/>
		<updated>2020-04-14T00:01:07Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* 2020-03-16 call summary: path forward on VERIFICATION paper */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi))&lt;br /&gt;
* Use RWG best source [https://scec.usc.edu/scecpedia/HighF_2018#Source_Models see 2020 updates here])&lt;br /&gt;
* Verify that best RG source is good at 15 stations for all models &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24190</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24190"/>
		<updated>2020-04-13T23:59:55Z</updated>

		<summary type="html">&lt;p&gt;Goulet: /* Related Pages */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi))&lt;br /&gt;
* Use RWG best source&lt;br /&gt;
* Verify that best RG source is good at 17 stations for all models &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12 High-F 14.12 description of parameters for verification and validation]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region (small domain)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24189</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24189"/>
		<updated>2020-04-13T23:56:06Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
&lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi))&lt;br /&gt;
* Use RWG best source&lt;br /&gt;
* Verify that best RG source is good at 17 stations for all models &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region]&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
	<entry>
		<id>https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24188</id>
		<title>HighF 2018</title>
		<link rel="alternate" type="text/html" href="https://strike.scec.org/scecwiki/index.php?title=HighF_2018&amp;diff=24188"/>
		<updated>2020-04-13T23:55:13Z</updated>

		<summary type="html">&lt;p&gt;Goulet: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This page documents the High-F activities and decisions for the 2018 verification and validation runs for three groups: Olsen et al. (AWP), Graves (RWG) and Taborda et al. (Hercules).&lt;br /&gt;
&lt;br /&gt;
== Mesh generation rules and parameter constraints ==&lt;br /&gt;
=== Domain definitions ===&lt;br /&gt;
Small domain: defined [https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region here]. &lt;br /&gt;
Large domain: defined [https://scec.usc.edu/scecpedia/HighF_v14.12#Simulation_Box_.2F_Velocity_Model here]. &lt;br /&gt;
&lt;br /&gt;
Use CVMS4.26.M01 (called cvmsi in UCVM, as per Table 1 in this [http://hypocenter.usc.edu/research/High-F_2020/Small_et_al_2017_SCEC_UCVM.pdf UCVM paper]), do NOT apply a GTL to the model, but apply the rules described below.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Velocities ===&lt;br /&gt;
* 1.	Set Min Vs=500 m/s&lt;br /&gt;
* 2.	If Vs was lower than 500 m/s and adjusted, then adjust Vp with original Vp/Vs ratio (so that we don’t have the automatic Vs/Vp of 3). We may want to set a minimum value of Vp (Rob to check)&lt;br /&gt;
* 3.	Then set Max Vp/Vs= 3, if  lower Vp to maintain the max of 3 ratio&lt;br /&gt;
&lt;br /&gt;
=== Lame parameters (mu and lambda) ===&lt;br /&gt;
Use mu and Lambda parameters to fix Vp/Vs issues in the CVM where necessary, as part of the mesh generation. Need to make sure that patches are physical and not only to make the codes run.&lt;br /&gt;
* Rob to check if raw model produces lambda of &amp;lt;=zero.&lt;br /&gt;
* Note: lambda of zero corresponds to Vp/Vs= sqrt(2)=1.45&lt;br /&gt;
* Note: typical Vp speeds are 330 m/s in air, 1450 m/s in water and about 5000 m/s in granite&lt;br /&gt;
&lt;br /&gt;
=== Anelastic attenuation (Q) ===&lt;br /&gt;
Frequency-independent Q definition&lt;br /&gt;
* Qs=100*Vs(km/s)&lt;br /&gt;
* Qp=2*Qs&lt;br /&gt;
&lt;br /&gt;
=== Upper frequency ===&lt;br /&gt;
&lt;br /&gt;
*  5Hz: based on 500 m/s and 20 m spacing&lt;br /&gt;
*  Kim and Rob have been low-pass filtering the slip function at 5 Hz&lt;br /&gt;
*  Ricardo and Naeem don’t filter the source&lt;br /&gt;
&lt;br /&gt;
== Source Models ==&lt;br /&gt;
We discussed various sources, both point source (PS) and finite-fault (FF) in the past for our verifications and validation. &lt;br /&gt;
* Various models were run in 2016:&lt;br /&gt;
** [https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison#Simulation_Results_-_22_May_2016 2016 runs with 2FF and 1 PS]&lt;br /&gt;
&lt;br /&gt;
* Also ran various smoothed variations of the GP15 FF (need to find a reference for that)&lt;br /&gt;
&lt;br /&gt;
* Rob to follow-up with Wei (last communication was in April 2017).&lt;br /&gt;
&lt;br /&gt;
Proposed models for verification and validation:&lt;br /&gt;
*PS: model from En-Jui (moment tensor). Can we replicate En-Jui's results? Would need to use CVMS4.26 (cms5) - not desirable. We could perform a check with CVS4.26.M01 at 5 sec. Need to use the same record En-Jui used. Proposed to use records from Figure 6 in:&lt;br /&gt;
** Lee E.-J., P. Chen, and T.H. Jordan (2014). Testing Waveform Predictions of 3D Velocity Models against Two Recent Los Angeles Earthquakes. Seismol. Res. Lett., 85 (6): 1275–1284 ([http://hypocenter.usc.edu/var/www/html/research/High-F_2018/Lee%2C%20Chen%2C%20Jordan%20-%202014%20-%20Testing%20Waveform%20Predictions%20of%203D%20Velocity%20Models%20against%20Two%20Recent%20Los%20Angeles%20Earthquakes.pdf Paper here])&lt;br /&gt;
*FF: [http://hypocenter.usc.edu/research/High-F_2018/LaHabra_notes-20170412-presented-2017-04-24.pdf Summary of agreed-upon FF model (gp.5.3.02)]&lt;br /&gt;
* FF refined with velocity model [http://hypocenter.usc.edu/research/High-F_2018/rwg_slides-20180221.pptx Slides from Graves presented on Feb. 21 2018]&lt;br /&gt;
&lt;br /&gt;
2020 updates:&lt;br /&gt;
* Revisiting finite fault selection for the verification paper&lt;br /&gt;
** Rob ran a series of tests to select a finite source to use with the Vmod floored at 500 m/s ([http://hypocenter.usc.edu/research/High-F_2020/source_nearfault-20200217.pptx powerpoint here])&lt;br /&gt;
** The suite of 40 SRF rupture models for the 2.5 km X 2.5 km fault are contained in this [http://hypocenter.usc.edu/research/High-F_2020/m5.14-2.5x2.5.tgz tarfile (364 MB)]. There are 2 resolutions: 100 m subfaults and 20m subfaults. The recommendation is to use 20m subfaults if possible.&lt;br /&gt;
&lt;br /&gt;
== Site Selection ==&lt;br /&gt;
2020 updates&lt;br /&gt;
* Step 1: fault model verification to be done by all groups, using the &amp;quot;small domain&amp;quot;, focused on near-by stations selected by Rob (need to link to text file here)&lt;br /&gt;
&lt;br /&gt;
== Simulation results ==&lt;br /&gt;
=== Results shared on March 5 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules, AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-03-05 AWP-Hercules-RWG Comparison With Observations]&lt;br /&gt;
&lt;br /&gt;
=== Results shared on March 12 2018 ===&lt;br /&gt;
Description: results for the small region from November 10 2017:&lt;br /&gt;
&lt;br /&gt;
Description: small region simulations for Hercules (updated to use simulations including Q), AWP (updated since November 2017) and RWG (medium size model to avoid boundary reflexions):&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Comparison]&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/bbp_comparison/awp-hercules-rwg-2018-03-12 AWP-Hercules-RWG Timeseries Comparison]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 2019-12-02 Call, summary of plans for 2020==&lt;br /&gt;
&lt;br /&gt;
=== Goals for 2020 === &lt;br /&gt;
** Verification paper (2020 Q1+?)&lt;br /&gt;
** Validation paper(s) (2020 Q2+?)&lt;br /&gt;
&lt;br /&gt;
=== Action items from call ===&lt;br /&gt;
* Rob to test other finite fault models using near-fault data and perform initial screening of candidate sources&lt;br /&gt;
* Christine to coordinate with Phil and Fabio for Jan. High-F sprint  &lt;br /&gt;
** to allow use of BBP GOF post-processors with high-f results and data&lt;br /&gt;
** to revive GOF map plotting tools (last run in 2016)&lt;br /&gt;
** Christine to verify that PSA results are ok (see anomaly on 20181125 results for observations of CE_13066). &lt;br /&gt;
** need to confirm start time as documented in post-processing code. Is it more or less constant with offset at all stations?&lt;br /&gt;
* Christine to re-start verification paper development&lt;br /&gt;
* Group need to document their submissions for point source or rerun them (see section below; finite fault is documented).&lt;br /&gt;
&lt;br /&gt;
=== Latest 2018 results documentation ===&lt;br /&gt;
Description: results for the small and large regions (model dependent) from November 10 2017, computed 20181125 using the latest ts_processor codes:&lt;br /&gt;
&lt;br /&gt;
* [http://hypocenter.usc.edu/bbp/highf/obs-awp-hercules-rwg-2018-11-25-vel/ AWP-Hercules-RWG-OBS Comparison]&lt;br /&gt;
&lt;br /&gt;
Summary documentation of extended source simulations submitted at [http://hypocenter.usc.edu/research/highf_data/ high-f]: &lt;br /&gt;
&lt;br /&gt;
Hercules 20171106 notes: &lt;br /&gt;
* Simulation of Mw 5.14 Lahabra Earthquake.(2014/03/29 04:09:42.97) with damping and using the extended source model provided by Robert Graves (downsampled version of the SRF for La Habra and based on 3D velocity model.The subfault spacing is 100 m). This simulation is part of High-F project. The simulation is done using the CVM-etree extracted from CVM-S4.26.M01 (28*28*14 km) at the “Small Domain.&amp;quot; See readme.txt in their folder for more info. &lt;br /&gt;
&lt;br /&gt;
RWG 20180425 notes: &lt;br /&gt;
* 20180425 - RWG simulation results for full-size model region (135 km x 180 km x 60 km). Velocity mesh was created on BlueWaters using UCVM interface that Scott C. created. Model is CVM-S4.26.M01 (at least I believe so, I selected 'cvmsi' as input to single_exe.py).  Vp/Vs capped at 3.0, Vsmin=500 ms, Qs=100*Vs(m/s), Qp=2*Qs. Time step is dt=0.001 sec.  Waveforms are ground velocity and have been low-pass filtered using zero-phase 4th order butterworth with corner at 5 Hz.&lt;br /&gt;
&lt;br /&gt;
AWP 20181203 notes:&lt;br /&gt;
* The latest anelastic simulation using cap of vp/vs=3, minimum Vs at 500 m/s with simulation length to 120 seconds in the large domain (180 km * 135 km * 60 km, grid spacing = 20 m). Number of stations: 351.&lt;br /&gt;
&lt;br /&gt;
== 2020-03-16 call summary: path forward on VERIFICATION paper ==&lt;br /&gt;
Verification of 5 Hz time series (4Hz PSA, multiple bands verification):	&lt;br /&gt;
* Use Vs floor of 500 m/s (CVMS4.26-M01 (cmvsi))&lt;br /&gt;
* Use RWG best source&lt;br /&gt;
* Verify that best RG source is good at 17 stations for all models &lt;br /&gt;
* Then all modelers rerun large region (need to confer on rotations before that step)&lt;br /&gt;
* Perform verification using results and plots from&lt;br /&gt;
** Seismtools&lt;br /&gt;
** tsprocess Anderson GOF scores and maps (GMT capability needs to be restored due to updates)&lt;br /&gt;
** BBP (GOF with T, distance, mapped, etc.; consider adding Vs30-based plots on BBP) &lt;br /&gt;
* Compare with 1D BBP sims (with Vs30=500 for all stations, with site response)?&lt;br /&gt;
* Write paper, publish&lt;br /&gt;
&lt;br /&gt;
== Related Pages ==&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/High-F_Project High-F Main page]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/HighF_v14.12_Data_Comparison Past verification (HighF_v14.12_Data)]&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulations_on_Titan La Habra simulations on Titan]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Simulation_Region La Habra Simulation region]&lt;br /&gt;
*[https://scec.usc.edu/scecpedia/La_Habra_Observational_Data La Habra Observational data]&lt;/div&gt;</summary>
		<author><name>Goulet</name></author>
		
	</entry>
</feed>