CyberShake Study 22.12

From SCECpedia
Jump to navigationJump to search

CyberShake Study 22.12 is a study in Southern California which includes deterministic low-frequency (0-1 Hz) and stochastic high-frequency (1-50 Hz) simulations. We used the Graves & Pitarka (2022) rupture generator and the high frequency modules from the SCEC Broadband Platform v22.4.


This study is complete. We are currently performing analysis of the results.

Data Products


Change from Study 15.4

Here's a table with the overall averaged differences between Study 15.4 and 22.12 at 2% in 50 years.

Negative difference and ratios less than 1 indicate smaller Study 22.12 results.

Period Difference (22.12-15.4) Ratio (22.12/15.4)
2 sec 0.0445 g 1.162
3 sec -0.00883 g 0.988
5 sec -0.0200 g 0.0901
10 sec -0.00846 0.882


Science Goals

The science goals for this study are:

  • Calculate a regional CyberShake model for southern California using an updated rupture generator.
  • Calculate an updated broadband CyberShake model.
  • Sample variability in rupture velocity as part of the rupture generator.
  • Increase hypocentral density, from 4.5 km to 4 km.

Technical Goals

The technical goals for this study are:

  • Use an optimized OpenMP version of the post-processing code.
  • Bundle the SGT and post-processing jobs to run on large Condor glide-ins, taking advantage of queue policies favoring large jobs.
  • Perform the largest CyberShake study to date.


We will use the standard 335 southern California sites (same as Study 21.12). The order of execution will be:

  • Stress test sites (site list here)
  • Sites of interest
  • 20 km grid
  • 10 km grid
  • Selected 5 km grid sites
Study 22.10 site map.png

Velocity Model

Summary: We are using a velocity model which is a combination of CVM-S4.26.M01 and the Ely-Jordan GTL:

  • At each mesh point in the top 700m, we calculate the Vs value from CVM-S4.26.M01, and from the Ely-Jordan GTL using a taper down to 700m.
  • We select the approach which produces the smallest Vs value, and we use the Vp, Vs, and rho from that approach.
  • We also preserve the Vp/Vs ratio, so if the Vs minimum of 500 m/s is applied, Vp will be scaled so the Vp/Vs ratio is the same.

We are planning to use CVM-S4.26 with a GTL applied, and the CVM-S4 1D background model outside of the region boundaries.

We are investigating applying the Ely-Jordan GTL down to 700 m instead of the default of 350m. We extracted profiles for a series of southern California CyberShake sites, with no GTL, a GTL applied down to 350m, and a GTL applied down to 700m.

Velocity Profiles

Sites (the CVM-S4.26 basins are outlined in red):

GTL profile sites.png

These are for sites outside of the CVM-S4.26 basins:

Site No GTL 700m GTL Smaller value, extracted from mesh 3 sec comparison curve
Study 15.4 w/no taper, Study 22.12 w/taper
Cvmsi default LAPD.png
Cvmsi elygtl ely z 700m LAPD.png
LAPD ifless profile.png
LAPD 3875 v 9538 3sec.png
Cvmsi default s764.png
Cvmsi elygtl ely z 700m s764.png
S764 ifless profile.png
S764 4248 v 9530 3sec.png
Cvmsi default s568.png
Cvmsi elygtl ely z 700m s568.png
S568 ifless profile.png
S568 4148 v 9489 3sec.png
Cvmsi default s035.png
Cvmsi elygtl ely z 700m s035.png
S035 ifless profile.png
S035 3981 v 9601 3sec.png
Cvmsi default PERR.png
Cvmsi elygtl ely z 700m PERR.png
PERR ifless profile.png
PERR 3951 v 9330 3sec.png
Cvmsi default MRVY.png
Cvmsi elygtl ely z 700m MRVY.png
MRVY ifless profile.png
MRVY 3920 v 9565 3sec.png
Cvmsi default s211.png
Cvmsi elygtl ely z 700m s211.png
S211 ifless profile.png
S211 4033 v 9435 3sec.png

These are for sites inside of the CVM-S4.26 basins:

Site No GTL 700m GTL Smaller value 3 sec comparison curve
Study 15.4 w/no taper, Study 22.12 w/taper
Cvmsi default s117.png
Cvmsi elygtl ely z 700m s117.png
S117 ifless profile.png
S117 4004 v 9415 3sec.png
Cvmsi default USC.png
Cvmsi elygtl ely z 700m USC.png
USC ifless profile.png
USC 3970 v 9306 3sec.png
Cvmsi default WNGC.png
Cvmsi elygtl ely z 700m WNGC.png
WNGC ifless profile.png
WNGC 3861 v 9314 3sec.png
Cvmsi default PEDL.png
Cvmsi elygtl ely z 700m PEDL.png
PEDL ifless profile.png
PEDL 3950 v 9336 3sec.png
Cvmsi default SBSM.png
Cvmsi elygtl ely z 700m SBSM.png
SBSM ifless profile.png
SBSM 3880 v 9320 3sec.png
Cvmsi default SVD.png
Cvmsi elygtl ely z 700m SVD.png
SVD ifless profile.png
SVD 4225 v 9647 3sec.png

Merged Taper Algorithm

Our algorithm for generating the velocity model, which we are calling the 'merged taper', is as follows:

  1. Set the surface mesh point to a depth of 25m.
  2. Query the CVM-S4.26.M01 model ('cvmsi' string in UCVM) for each grid point.
  3. Calculate the Ely taper at that point using 700m as the transition depth. Note that the Ely taper uses the Thompson Vs30 values in constraining the taper near the surface.
  4. Compare the values before and after the taper modification; at each grid point down to the transition depth, use the value from the method with the lower Vs value.
  5. Check values for Vp/Vs ratio, minimum Vs, Inf/NaNs, etc.

Value constraints

We impose the following constraints (in this order) on velocity mesh values. The ones in bold are new for Study 22.12.

  1. Vs >= 500 m/s. If lower, Calculate the Vp/Vs ratio. Set Vs=500, and Vp=Vs*(Vp/Vs ratio) [which in this case is Vp=500*(Vp/Vs ratio)].
  2. Vp >= 1700 m/s. If lower, Vp is set to 1700.
  3. rho = 1700 km/m3. If lower, rho is set to 1700.
  4. Vp/Vs >= 1.45. If not, Vs is set to Vp/1.45.


Below are cross-sections of the TEST site velocity model at depths down to 600m for CVM-S4.26.M01, the taper to 700m, the lesser of the two values, and the % difference.

Note that the top two slices use a different color scale.

Depth CVM-S4.26.M01 Ely taper to 700m Selecting smaller value % difference, smaller value vs S4.26.M01
0m (queried at 25m depth)
TEST none horiz z0.png
TEST all horiz z0.png
TEST ifless horiz z0.png
TEST percentdiff horiz z0.png
TEST none horiz z1.png
TEST all horiz z1.png
TEST ifless horiz z1.png
TEST percentdiff horiz z1.png
TEST none horiz z2.png
TEST all horiz z2.png
TEST ifless horiz z2.png
TEST percentdiff horiz z2.png
TEST none horiz z3.png
TEST all horiz z3.png
TEST ifless horiz z3.png
TEST percentdiff horiz z3.png
TEST none horiz z4.png
TEST all horiz z4.png
TEST ifless horiz z4.png
TEST percentdiff horiz z4.png
TEST none horiz z5.png
TEST all horiz z5.png
TEST ifless horiz z5.png
TEST percentdiff horiz z5.png
TEST none horiz z6.png
TEST all horiz z6.png
TEST ifless horiz z6.png
TEST percentdiff horiz z6.png

Implementation details

To support the Ely taper approach where the smaller value is selected, the following algorithmic changes were made to the CyberShake mesh generation code. Since the UCVM C API doesn't support removing models, we couldn't just add the 'elygtl' model - it would then be included in every query, and we need to run queries with and without it to make the comparison. We also must include the Ely interpolator, since all that querying the elygtl model does is populates the gtl part of the properties with the Vs30 value, and it's the interpolator which takes this and the crustal model info and generates the taper.

  • The decomposition is done by either X-parallel or Y-parallel stripes, which have a constant depth. Check the depth to see if it is shallower than the transition depth.
  • If so, initialize the elygtl model using ucvm_elygtl_model_init(), if uninitialized. Set the id to UCVM_MAX_MODELS-1. There's no way to get model id info from UCVM, so we use UCVM_MAX_MODELS-1 as it is 29, we are very unlikely to load 29 models, and therefore unlikely to have an id conflict.
  • Change the depth value of the points to query to the transition depth. This is because we need to know the crustal model Vs value at the transition depth, so that the Ely interpolator can match it.
  • Query the crustal model again, with the modified depths.
  • Modify the 'domain' parameter in the properties data structure to UCVM_DOMAIN_INTERP, to indicate that we will be using an interpolator.
  • Change the depth value of the points to query back to the correct depth, so that the interpolator can work correctly on them.
  • Query the elygtl using ucvm_elygtl_model_query() and the correct depth.
  • Call the interpolator for each point independently, using the correct depth.
  • For each point, choose to use either the original crustal data or the Ely taper data, depending on which has the lower Vs.

In the future we plan for this approach to be implemented in UCVM, and we can simplify the CyberShake query code.

Impact on hazard

Below are hazard curves calculated with the old approach, and with the implementation described above, for WNGC.

black=using CVM-S4.26.M01,blue=using approach with smaller Vs
black=using CVM-S4.26.M01,blue=using approach with smaller Vs
black=using CVM-S4.26.M01,blue=using approach with smaller Vs
black=using CVM-S4.26.M01,blue=using approach with smaller Vs

These are scatterplots for the above WNGC curves.

black=using CVM-S4.26.M01,blue=using approach with smaller Vs
black=using CVM-S4.26.M01,blue=using approach with smaller Vs
black=using CVM-S4.26.M01,blue=using approach with smaller Vs
black=using CVM-S4.26.M01,blue=using approach with smaller Vs

Velocity Model Info

For Study 22.12, we track and use a number of velocity model-related parameters, in the database and as input to the broadband codes. Below we track where values come from and how they are used.

Broadband codes

  • The code that is used to calculate high-frequency seismograms takes three parameters: vs30, vref, and vpga. vref and vpga are 500 m/s. Vs30 comes from the 'Target_Vs30' parameter in the database, which itself comes from the Thompson et al. (2020) model.
  • The low-frequency site response code also has three parameters: vs30, vref, and vpga. Vs30 also comes from the 'Target_Vs30' parameter in the database, which itself comes from the Thompson (2020) model. Vref is calculated as ('Model_Vs30' database parameter) * (VsD500)/(Vs500). Vpga is 500.0.
    • Model_Vs30 is calculated using a slowness average of the top 30 m from UCVM.
    • VsD500 is the slowness average of the grid points at the surface, 100m, 200m, 300m, 400m, and 500m depth. Note that for this study, the surface grid point is populated by querying UCVM at a depth of 25m.
    • Vs500 is the slowness average of the top 500m from UCVM.

Database values

The following values related to velocity structure are tracked in the database:

  • Model_Vs30: This Vs30 value is calculated by taking a slowness average at 1-meter increments from [0.5, 29.5] and querying UCVM, with the merged taper applied. This value is populated in low-frequency runs, and copied over to the corresponding broadband run.
  • Mesh_Vsitop_ID: This identifies what algorithm was used to populate the surface grid point. For Study 22.12, we query the model at a depth of (grid spacing/4), or 25m.
  • Mesh_Vsitop: The value of the surface grid point at the site, populated using the algorithm specified in Mesh_Vsitop_ID.
  • Minimum_Vs: Minimum Vs value used in generating the mesh. For Study 22.12, this is 500 m/s.
  • Wills_Vs30: Wills Vs30 value. Currently this parameter is unpopulated.
  • Z1_0: Z1.0 value. This is calculated by querying UCVM with the merged taper at 10m increments. If there is more than one crossing of 1000 m/s, we select the second crossing. If there is only 1 crossing, we use that.
  • Z2_5: Z2.5 value. This is calculated by querying UCVM with the merged taper at 10m increments. If there is more than one crossing of 2500 m/s, we select the second crossing. If there is only 1 crossing, we use that.
  • Vref_eff_ID: This identifies the algorithm used to calculate the effective vref value used in the low-frequency site response. For Study 22.12, it is Model_Vs30 * VsD500/Vs500.
  • Vref_eff: This is the value obtained when following the algorithm identified in Vref_eff_ID
  • Vs30_Source: Source of the Target_Vs30 value. For Study 22.12, this is Thompson et al. (2020)
  • Target_Vs30: This is the value used for Vs30 when performing site response. It's populated using the source in Vs30_Source.

Rupture Generator

Summary: We are using the Graves & Pitarka generator v5.5.2, the same version as used in the BBP v22.4, for Study 22.12.

Initial Findings

In determining what rupture generator to use for this study, we performed tests with WNGC, USC, PAS, and STNI, and compared hazard curves generated with v5.4.2 to those from Study 15.4:

Site 10 sec 5 sec 3 sec 2 sec
WNGC run8685 v 3861 10sec.png
WNGC run8685 v 3861 5sec.png
WNGC run8685 v 3861 3sec.png
WNGC run8685 v 3861 2sec.png
USC run8691 v 3970 10sec.png
USC run8691 v 3970 5sec.png
USC run8691 v 3970 3sec.png
USC run8691 v 3970 2sec.png
PAS run8687 v 3878 10sec.png
PAS run8687 v 3878 5sec.png
PAS run8687 v 3878 3sec.png
PAS run8687 v 3878 2sec.png
STNI run8689 v 3873 10sec.png
STNI run8689 v 3873 5sec.png
STNI run8689 v 3873 3sec.png
STNI run8689 v 3873 2sec.png

Digging in further, it appears the elevated hazard curves for WNGC at 2 and 3 seconds are predominately due to large-magnitude southern San Andreas events producing larger ground motions.

Scatter plot comparing the mean 3sec RotD50 for each rupture, between v3.3.1 and v5.4.2
Scatter plot comparing the mean 3sec RotD50 for each rupture, between v3.3.1 and v5.4.2, SAF events>M8 excluded
Scatter plot comparing the mean 3sec RotD50 for each rupture, between v3.3.1 and v5.4.2, SAF events>M7.5 excluded

USC, PAS, and STNI also all see larger ground motions at 2-3 seconds from these same events, but the effect isn't as strong, so it only shows up in the tails of the hazard curves.

We honed in on source 68, rupture 7, a M8.45 on the southern San Andreas which produced the largest WNGC ground motions at 3 seconds, up to 5.1g. We calculated spectral plots for v3.3.1 and v5.4.2 for all 4 sites:

Site v3.3.1 v5.4.2
WNGC 3861 v3.3.1 spectral s68 r7.png
WNGC 8685 v5.4.2 spectral s68 r7.png
USC 3970 v3.3.1 spectral s68 r7.png
USC 8691 v5.4.2 spectral s68 r7.png
PAS 3878 v3.3.1 spectral s68 r7.png
PAS 8687 v5.4.2 spectral s68 r7.png
STNI 3873 v3.3.1 spectral s68 r7.png
STNI 8689 v5.4.2 spectral s68 r7.png


We decided to try v5.5.2 of the rupture generator, which typically has less spectral content at short periods:

Site v3.3.1 v5.4.2 v5.5.2
WNGC 3861 v3.3.1 spectral s68 r7.png
WNGC 8685 v5.4.2 spectral s68 r7.png
WNGC 8693 v5.5.2 spectral s68 r7.png

Hazard Curves

Comparison hazard curves for the three rupture generators, using no taper

Site 10 sec 5 sec 3 sec 2 sec
WNGC rg compare 10sec.png
WNGC rg compare 5sec.png
WNGC rg compare 3sec.png
WNGC rg compare 2sec.png
USC rg compare notaper 10sec.png
USC rg compare notaper 5sec.png
USC rg compare notaper 3sec.png
USC rg compare notaper 2sec.png

Comparison curves for the three rupture generators, using the smaller value in the velocity model.

Site 10 sec 5 sec 3 sec 2 sec
STNI rg compare taper 10sec.png
STNI rg compare taper 5sec.png
STNI rg compare taper 3sec.png
STNI rg compare taper 2sec.png
PAS rg compare taper 10sec.png
PAS rg compare taper 5sec.png
PAS rg compare taper 3sec.png
PAS rg compare taper 2sec.png

Scatter Plots

Scatter plots, comparing results with v5.5.2 to results from Study 15.12 by plotting the mean ground motion for each rupture. The colors are magnitude bins (blue: <M6.5; green: M6.5-7; yellow: M7-7.5; orange: M7.5-8; red: M8+).

Site 10 sec 5 sec 3 sec 2 sec
WNGC 8694 v 4293 scatter 10sec.png
WNGC 8694 v 4293 scatter 5sec.png
WNGC 8694 v 4293 scatter 3sec.png
WNGC 8694 v 4293 scatter 2sec.png
PAS 8700 v 4282 scatter 10sec.png
PAS 8700 v 4282 scatter 5sec.png
PAS 8700 v 4282 scatter 3sec.png
PAS 8700 v 4282 scatter 2sec.png
USC 8698 v 4384 scatter 10sec.png
USC 8698 v 4384 scatter 5sec.png
USC 8698 v 4384 scatter 3sec.png
USC 8698 v 4384 scatter 2sec.png
STNI 8702 v 4285 scatter 10sec.png
STNI 8702 v 4285 scatter 5sec.png
STNI 8702 v 4285 scatter 3sec.png
STNI 8702 v 4285 scatter 2sec.png

We also modified the risetime_coef to 2.3, from the previous default of 1.6.

High-frequency codes

For this study, we will use the Graves & Pitarka high frequency module (hb_high) from the Broadband Platform v22.4, hb_high_v6.0.5. We will use the following parameters. Parameters in bold have been changed for this study.

Parameter Value
stress_average 50
rayset 2,1,2
siteamp 1
nbu 4 (not used)
ifft 0 (not used)
flol 0.02 (not used)
fhil 19.9 (not used)
irand Seed used for generating SRF
tlen Seismogram length, in sec
dt 0.01
fmax 10 (not used)
kappa 0.04
qfexp 0.6
mean_rvfac 0.775
range_rvfac 0.1
rvfac Calculated using BBP code
shal_rvfac 0.6
deep_rvfac 0.6
czero 2
c_alpha -99
sm -1
vr -1
vsmoho 999.9
nlskip -99
vpsig 0
vshsig 0
rhosig 0
qssig 0
icflag 1
velname -1
fa_sig1 0
fa_sig2 0
rvsig1 0.1
ipdur_model 11
ispar_adjust 1
targ_mag -1
fault_area -1
default_c0 57
default_c1 34

Spectral Content around 1 Hz

We investigated the spectral content of the Broadband CyberShake results in the 0.5-3 second range, to look for any discontinuities.

The plot below is from WNGC, Study 15.12 (run ID 4293).

Spectral plot for WNGC from Study 15.12, target of 0.3676g @ 3 sec. Mean is in red.

Below is a plot of the hypocenters from the 706 rupture variations which meet the target.

WNGC run4293 target event hypos.png

These events have a different distribution than the rupture variations as a whole.

Fault Percent of target RVs Percent of all RVs
San Andreas 60 44
Elsinore 21 9
San Jacinto 13 8
Other 6 39

Additionally, 88% of the selected events have a magnitude greater than the average for their source. 4% are average, and 8% are lower.

Below is a spectral plot but which includes all rupture variations and the overall mean (in orange).

Spectral plot for WNGC from Study 15.12, all variations.

Additional Sites

We created spectral plots for 7 additional sites (STNI, SBSM, PAS, LGU, LBP, ALP, PLS), located here:

Additional spectral plot sites.png
STNI run4285 full spectra.png
SBSM run4291 full spectra.png
PAS run4282 full spectra.png
LGU run4321 full spectra.png
LBP run4317 full spectra.png
ALP run4298 full spectra.png
PLS run4370 full spectra.png


We created spectral plots using results produced with rupture generator v5.5.2. These results have a much less noticeable slope around 1 sec.

WNGC run8694 full spectra.png
PAS run8700 full spectra.png
USC run8698 full spectra.png
STNI run8702 full spectra.png

Seismogram Length

Originally we proposed a seismogram length of 500 sec. We examined seismograms for our most distance event-station pairs for this study and concluded that most stop having any meaningful signal by around 325 sec. Thus, we are reducing the seismogram length to 400 sec to ensure some margin of error.


The extensive validation efforts performed in preparation for this study are documented in Broadband_CyberShake_Validation.

Updates and Enhancements

  • New velocity model created, including Ely taper to 700m and tweaked rules for applying minimum values.
  • Updated to rupture generator v5.5.2.
  • CyberShake broadband codes now linked directly against BBP codes
  • Added -ffast-math compiler option to hb_high code for modest speedup.
  • Migrated to using OpenMP version of DirectSynth code.
  • Optimized rupture generator v5.5.2.
  • Verification was performed against historic events, including Northridge and Landers.

Lessons Learned from Previous Studies

  • Create new velocity model ID for composite model, capturing metadata.
  • We created a new velocity model ID to capture the model used for Study 22.12.
  • Clear disk space before study begins to avoid disk contention.
  • On moment, we migrated old studies to focal and optimized. At CARC, we migrated old studies to OLCF HPSS.
  • In addition to disk space, check local inode usage.
  • CARC and shock checked; plenty of inodes are available.

Output Data Products

File-based data products

We plan to produce the following data products, which will be stored at CARC:


  • Seismograms: 2-component seismograms, 8000 timesteps (400 sec) each.
  • PSA: X and Y spectral acceleration at 44 periods (10, 9.5, 9, 8.5, 8, 7.5, 7, 6.5, 6, 5.5, 5, 4.8, 4.6, 4.4, 4.2, 4, 3.8, 3.6, 3.4, 3.2, 3, 2.8, 2.6, 2.4, 2.2, 2, 1.66667, 1.42857, 1.25, 1.11111, 1, .66667, .5, .4, .33333, .285714, .25, .22222, .2, .16667, .142857, .125, .11111, .1 sec)
  • RotD: PGV, and RotD50, the RotD50 azimuth, and RotD100 at 25 periods (20, 15, 12, 10, 8.5, 7.5, 6.5, 6, 5.5, 5, 4.4, 4, 3.5, 3, 2.8, 2.6, 2.4, 2.2, 2, 1.7, 1.5, 1.3, 1.2, 1.1, 1)
  • Durations: for X and Y components, energy integral, Arias intensity, cumulative absolute velocity (CAV), and for both velocity and acceleration, 5-75%, 5-95%, and 20-80%.


  • Seismograms: 2-component seismograms, 40000 timesteps (400 sec) each.
  • PSA: X and Y spectral acceleration at 44 periods (10, 9.5, 9, 8.5, 8, 7.5, 7, 6.5, 6, 5.5, 5, 4.8, 4.6, 4.4, 4.2, 4, 3.8, 3.6, 3.4, 3.2, 3, 2.8, 2.6, 2.4, 2.2, 2, 1.66667, 1.42857, 1.25, 1.11111, 1, .66667, .5, .4, .33333, .285714, .25, .22222, .2, .16667, .142857, .125, .11111, .1 sec)
  • RotD: PGA, PGV, and RotD50, the RotD50 azimuth, and RotD100 at 66 periods (20, 15, 12, 10, 8.5, 7.5, 6.5, 6, 5.5, 5, 4.4, 4, 3.5, 3, 2.8, 2.6, 2.4, 2.2, 2, 1.7, 1.5, 1.3, 1.2, 1.1, 1, 0.85, 0.75, 0.65, 0.6, 0.55, 0.5, 0.45, 0.4, 0.35, 0.3, 0.28, 0.26, 0.24, 0.22, 0.2, 0.17, 0.15, 0.13, 0.12, 0.11, 0.1, 0.085, 0.075, 0.065, 0.06, 0.055, 0.05, 0.045, 0.04, 0.035, 0.032, 0.029, 0.025, 0.022, 0.02, 0.017, 0.015, 0.013, 0.012, 0.011, 0.01)
  • Durations: for X and Y components, energy integral, Arias intensity, cumulative absolute velocity (CAV), and for both velocity and acceleration, 5-75%, 5-95%, and 20-80%.

Database data products

We plan to store the following data products in the database on moment:


  • RotD50 and RotD100 for 6 periods (10, 7.5, 5, 4, 3, 2)
  • Duration: acceleration 5-75% and 5-95%, for both X and Y


  • RotD50 and RotD100 for PGA, PGV, and 19 periods (10, 7.5, 5, 4, 3, 2, 1, 0.75, 0.5, 0.4, 0.3, 0.2, 0.1, 0.075, 0.05, 0.04, 0.03, 0.02, 0.01)
  • Duration: acceleration 5-75% and 5-95%, for both X and Y

Computational and Data Estimates

Computational Estimates

We based these estimates on scaling from the average of sites USC, STNI, PAS, and WNGC, which have within 1% of the average number of variations per site.

SGT calculation
UCVM runtime UCVM nodes SGT runtime (both components) SGT nodes Other SGT workflow jobs Summit Total
4 site average 436 sec 50 3776 sec 67 8700 node-sec 78.8 node-hrs

78.8 node-hrs x 335 sites + 10% overrun margin gives us an estimate of 29.0k node-hours for SGT calculation.

PP calculation, with the OpenMP optimization
DirectSynth runtime DirectSynth nodes Summit Total
4 site average 31000 92 792

792 node-hours x 335 sites + 10% overrun margin gives an estimate of 292k node-hours for post-processing.

Broadband calculation
PMC runtime PMC nodes Summit Total
4 site average 31500 92 805

805 node-hrs x 335 sites + 10% overrun margin gives an estimate of 297k node-hours for broadband calculations.

Data Estimates


On average, each site contains 626,000 rupture variations.

These estimates assume a 400 sec seismogram.

Data estimates
Velocity mesh SGTs size Temp data Output data
4 site average (GB) 177 1533 1533 225
Total for 335 sites (TB) 57.8 501.4 501.4 73.6


We estimate 225.6 GB/site x 335 sites = 73.8 TB in output data, which will be transferred back to CARC. After transferring Study 13.4 and 14.2, we have 66 TB free at CARC, so additional data will need to be moved.


The study should use approximately 737 GB in workflow log space on /home/shock. This drive has approximately 1.5 TB free.

moment database

The PeakAmplitudes table uses approximately 99 bytes per entry.

99 bytes/entry * 34 entries/event (11 det + 25 stoch) * 622,636 events/site * 335 sites = 654 GB. The drive on moment with the mysql database has 771 GB free, so we will plan to migrate Study 18.8 off of moment to free up additional room.

Lessons Learned

  • Make sure database space estimates include both RotD50 and RotD100 values, and also include the space required for indices.
  • Add sanity checks on all intensity measures inserted, not just the geometric means (which aren't being inserted anymore).
  • Test all types of bundled glidein jobs before the production run. (The AWP jobs ran fine, but we had issues with the DirectSynth jobs).
  • Make sure all appropriate velocity fields in the DB are being populated.
  • Come up with a solution to the out/err file issue with the BB runs. With file-per-worker, PMC gets a seg fault when the final output is combined. With file-per-task, we end up with 160k files and the filesystem becomes angry.

Stress Test

As of 12/17/22, user callag has run 13627 jobs and consumed 71936.9 node-hours on Summit.

/home/shock on shock-carc has 1544778288 blocks free.

The stress test started at 15:47:42 PST on 12/17/22.

The stress test completed at 13:32:20 PST on 1/7/23, for an elapsed time of 501.7 hours.

As of 1/10/23, user callag has run 14204 jobs and consumed 115430.8 node-hours on Summit.

This works out to 2174.7 node-hours per site, 29.7% more than the initial estimate of 1675.8.

Issues Discovered

  • The cronjob submission script on shock-carc was assigning Summit as the SGT and PP host, meaning that summit-pilot wasn't considered in planning.

We removed assignment of SGT and PP host at workflow creation time.

  • Pegasus was trying to transfer some files from CARC to shock-carc /tmp. Since CARC is accessed via the GO protocol, but /tmp isn't served through GO, there doesn't seem to be a way to do this.

Reverted to custom pegasus-transfer wrapper until Pegasus group can modify Pegasus so that files aren't transferred to /tmp which aren't used in the planning process. This will probably be some time in January.

  • Runtimes for DirectSynth jobs are much slower (over 10 hours) than in testing.

Increased the permitted memory size from 1.5 GB to 1.8 GB, to reduce the number of tasks and (hopefully) get better data reuse.

  • Velocity info job, which determines Vs30, Vs500, and VsD500 for site correction, doesn't apply the taper when calculating these values.

Modified the velocity info job to use the taper when calculating various velocity parameters.

  • Velocity params job, which populated the database with Vs30, Z1.0, and Z2.5, doesn't apply the taper.

Modified the velocity params job to use the taper.

  • Velocity parameters aren't being added to the broadband runs, just the low-frequency runs.

Added a new job to the DAX generator to insert the Vs30 value from the velocity info file, and copy Z1.0 and Z2.5 from the low-frequency run.

  • Minimum Vs value isn't being added to the DB.

Modified the Run Manager to insert a default minimum Vs value of 500 m/s in the DB when a new run is created.

Events During Study

  • For some reason (slow filesystem?), several of the serial jobs, like PreCVM and PreSGT, kept failing due to wallclock time expiration. I adjusted the wallclock times up to avoid this.
  • In testing, runtimes for the AWP_SGT jobs were around 35 minutes, so we set our pilot job run times to 40 minutes. However, this was not enough time for the AWP_SGT jobs during production, so the work would start over with every pilot job. We increased runtime to 45 minutes, but that still wasn't enough for some jobs, so we increased it again to 60 minutes. This comes at the cost of increased overhead, since the time between the end of the job and the hour is basically lost, but it is better than having jobs never finish.
  • We finished the SGT calculations on 1/26.
  • On 2/1 we found and fixed an issue with the OpenSHA calculation of locations, which resulted in a mismatch between the CyberShake DB source ID/rupture ID and the source ID/rupture ID in OpenSHA. This affected scatterplots and disaggregation calculations, so all disagg calcs done before this date need to be redone.
  • On 2/2 we found that the DirectSynth jobs running in the pilot jobs which are bundled into 10 are segfaulting within the first ~10 sec, before any log files are written. We confirmed this issue doesn't happen with the single-node glidein jobs, and reverted back to those. We will try tests with bundles of 2 jobs to see if we can identify the issue.
  • We started getting excellent throughput during the week of 1/30. So as not to use up the allocation, we paused deterministic post-processing calculations on 2/8. We got approval to 2/10 to continue running without penalty, and resumed the deterministic post-processing then.
  • We finished the deterministic calculations on 2/22.
  • On 2/27, we got an email from OLCF about excessive load from the BB jobs on the GPFS filesystem. We are writing more files with the BB jobs - about 150k per run - but a bigger issue may be the file-per-task I/O that we turned on, increasing the number of err & out files from 6k to 160k. We turned that on to try to prevent the segfaults we were seeing when the workflow finished and the manager was trying to merge all the I/O back in. However, we may need to take that hit so we can maintain a higher number of jobs. Currently OLCF has reduced us to 4 simultaneous jobs, which means it will take about 2 weeks to finish up the BB runs.
  • Looking at the initial hazard map, we identified 3 sites with way-too-low ground motions. Digging in, all the RotD values are O(1e-30). This is because the SGTs were not transferred correctly, and even though the check jobs failed, the DirectSynth job ran, the files were transferred back to CARC, the data was inserted into the DB, and curves were generated. The check that we have on the intensity measures upon insertion is only for the geometric mean values, so this should be added to the RotD values as well.
  • The broadband calculations finished on 3/6, with the rerun of s003. We just have the DB insertions for about 70% of the BB runs remaining.

Database Space Issue

On 2/23, we began noticing the free space on moment rapidly disappearing. In 24 hours it was reduced from 310 GB to 140 GB, with still about 75% of the broadband runs remaining.

Additionally, this coincided with many errors with inserting data. What we see happening is that the loading of amplitudes aborts after awhile, but doesn't return an error. Then, when the check job runs, not all the needed rupture variations are present, and the workflow aborts at this step.

The space issue happened because we made two mistakes when calculating the data size. The first is that we did not take into account the size of the indices for each entry in the PeakAmplitudes table, which is about the same size as the data itself. The second is that we forgot that we were also inserting RotD100 values for all 21 broadband periods, not just RotD50, so that's another factor of 2.

With these new values, data + index sizes for the PeakAmplitudes table average 269 bytes/row. Each broadband run has about 620k rupture variations, and we're inserting 21 periods * 2 RotD values + 4 durations for each variation. This works out to 269 bytes/IM * 46 IMs/variation * 622k variations/site = 7.2 GB/site, or 2.4 TB for the entire study.


The immediate issues are:

  1. Failed database insertions are preventing sites from finishing.
  2. Moment will run out of space before the study completes.

These are the planned steps to be able to resume the study:

  1. Pause the broadband runs.
  2. Create a cronjob on shock-carc which will kill workflows when they hit the Load_Amps stage. This will avoid using extra space on the DB, but will make it easy to resume once more space is freed.
  3. Restart broadband workflows, knowing they'll be stopped when they get to the database stage.

Ultimately, we need to populate moment to be able to support access and comparisons. Currently, we need 1800 GB and we have 100 GB.

  1. Drop Study 17.3 from the PeakAmps table. This study has 4.5 billion rows. There is some uncertainty about how much space this will free up, but it's a minimum of 1140 GB. This increases our available space to 1240 GB.
  2. Assess how much space is available. If more space is required, consider dropping some of the test runs in the DB which we no longer need.
  3. Remove cronjob which kills workflows in Load_Amps stage.
  4. Restart workflows which were stopped at Load_Amps stage.
  5. Clean up and restart workflows with database insertion issues.

On 3/12, we ran out of database space with 93 sites remaining to be inserted, about 670 GB.

  1. I reduced the size of the 2 log files from 2 GB to 1 GB, freeing up 2 GB on the database disk.
  2. I created a temporary file 1 GB in size, so we could delete in in the future and have a little breathing room.
  3. I switched MariaDB's temporary space from /export/moment, which is basically full, to /tmp, which has about 60 GB of space.
  4. Since Study 15.12 has already been migrated to focal, we will delete Study 15.12 off moment. This should free up approximately 1460 GB, which should be plenty of space. We could consider stopping after about 200 deleted sites to speed up inserts.
  5. We will then restart workflow population.
  6. Once the study is complete, we will attach a temporary drive of 500 GB - 1 TB to moment to use as mysql temp, and then run optimize table to clean up the fragmentation and get back disk space.
  7. Once disk space is reclaimed, the temporary drive can be removed and we can begin migrating data into sqlite databases and moment-carc.


On 2/24, moment has 134 GB free. We've stopped running new workflows and are just letting the ones currently running finish.

We began the Study 17.3 deletions the evening of 2/24. We expect they will take about a week.

We resumed the workflows the evening of 2/24, with a cronjob on shock to kill workflows when they hit the Load_Amps stage. This is for workflows starting with ID 9896

On 2/27, we started cleaning up the runs which had incomplete inserts.

The Study 17.3 deletions finished on 3/3. We then ran 'analyze table' to see if that updates the information_schema info, but it didn't. Based on the number of rows deleted, we estimate we've freed around 1100 GB.

On 3/4, we queued up deletions of all the runs with incomplete inserts.

On 3/12, we ran out of disk space on moment, with about 25% of the broadband runs remaining to be inserted. We started deleting Study 15.12 off moment. To give it a head start, we found some runs which haven't finished their BB processing, so we turned back on the cronjob which kills workflows at the LoadAmps stage and are resuming the BB processing for these jobs.

Performance Metrics

At the start of the main study, user callag had run 14466 jobs and used 116506.7 node-hours on the GEO112 allocation on Summit.

The main study began on 1/17/23 at 22:34:11 PST.

The main study ended on 4/4/23 at 04:46:40 PDT, for a main study elapsed time of 1829.2 hours.

At the end of the main study, user callag had run 25320 jobs and used 845339.1 node-hours on the GEO112 allocation.

Application Level Metrics

  • We ran a total of 965 top-level workflows: 20 for the stress test sites + 3*315 for the other sites.
  • We ran 20*83 + 315*(26+27+31) = 28,120 jobs successfully (retries are tracked elsewhere).
    • Integrated workflow: 10 jobs (3 dir create, 1 stage) + AWP + PreDS + DS + BB + 2*DB + post = 83
    • SGT workflow: 6 jobs (2 dir create, 1 stage) + AWP = 26
    • PP workflow: 1 job (1 dir create) + PreDS + DS + Post + DB = 27
    • Stoch workflow: 8 jobs (3 dir create, 1 stage) + BB + DB + Post = 31
    • AWP subworkflow: 20 jobs (2 dir create, 3 stage, 2 register)
    • PreDS subworkflow: 7 jobs (2 dir create, 1 stage)
    • DS subworkflow: 6 jobs (1 dir create, 3 stage, 2 register)
    • BB subworkflow: 10 jobs (2 dir create, 3 stage, 1 register)
    • DB subworkflow: 10 jobs (2 dir create)
    • Post subworkflow: 3 jobs (1 dir create)

Production Checklist

Science to-dos

  • Run WNGC and USC with updated velocity model.
  • Redo validation for Northridge and Landers with updated velocity model, risetime_coef=2.3, and hb_high v6.1.1.
  • For each validation event, calculate BBP results, CS results
  • Check for spectral discontinuities around 1 Hz
  • Decide if we should stick with rvfrac=0.8 or allow it to vary
  • Determine appropriate SGT, low-frequency, and high-frequency seismogram durations
  • Update high-frequency Vs30 to use released Thompson values
  • Modify RupGen-v5.5.2 into CyberShake API
  • Test RupGen-v5.5.2
  • Update to using v6.1.1 of hb_high.
  • Add metadata to DB for merged taper velocity model.
  • Check boundary conditions.
  • Check that Te-Yang's kernel fix is being used.

Technical to-dos

  • Integrate refactoring of BBP codes into latest BBP release
  • Switch to using github repo version of CyberShake on Summit
  • Update to latest UCVM (v22.7)
  • Switch to optimized version of rupture generator
  • Test DirectSynth code with fixed memory leak from Frontera
  • Switch to using Pegasus-supported interface to Globus transfers.
  • Test bundled glide-in jobs for SGT and DirectSynth jobs
  • Fix seg fault in PMC running broadband processing
  • Update curve generation to generate curves with more points
  • Test OpenMP version of DirectSynth
  • Migrate Study 18.8 from moment to focal.
  • Delete Study 18.8 off of moment.
  • Optimize PeakAmplitudes table on moment.
  • Move Study 13.4 output files from CARC to OLCF HPSS.
  • Move Study 14.2 output files from CARC to OLCF HPSS.
  • Switch to using OMP version of DS code by default.
  • Review wiki content.
  • Switch to using Python 3.9 on shock.
  • Confirm PGA and PGV are being calculated and inserted into the DB.
  • Drop rupture variations and seeds tables for RV ID 9, in case we need to put back together for SQLite running.
  • Change to Pegasus 5.0.3 on shock-carc.
  • Tag code.

Presentations, Posters, and Papers

Science Readiness Review

Technical Readiness Review


Details about the Graves & Pitarka stochastic approach used in the SCEC Broadband Platform, v22.4, the same as is used in this study: [1]

The merged taper was based off work by Hu, Olsen, and Day showing that a 700-1000m taper improves the fit between synthetics and data for La Habra: [2]