Difference between revisions of "Moved:SCEC UGMS Committee Meeting 6"
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== Data == | == Data == | ||
| − | We have extracted timeseries data for the following | + | We have extracted timeseries data for the following 4 events: |
#Southern San Andreas, nucleating near Bombay Beach (33.3772, -115.74, 4.1514 km deep): source 59, rupture 3, rupture variation 0.<br/>Plots available [http://hypocenter.usc.edu/research/cybershake/5_16_UGMS_Meeting/timeseries/SAF_Coachella here]. | #Southern San Andreas, nucleating near Bombay Beach (33.3772, -115.74, 4.1514 km deep): source 59, rupture 3, rupture variation 0.<br/>Plots available [http://hypocenter.usc.edu/research/cybershake/5_16_UGMS_Meeting/timeseries/SAF_Coachella here]. | ||
Revision as of 17:39, 15 April 2016
- SCEC Committee for Utilization of Ground Motion Simulations Meeting 6
- Organizers: C.B. Crouse (AECOM) and Tom Jordan (SCEC/USC)
- Date: Monday, May 16, 2016 (10:00-15:00)
- Location: SCEC Board Room (ZHS 167), USC, Los Angeles, CA
- Participants: TBD (by invitation only)
Agenda
Presentation slides may be downloaded by clicking each title. PLEASE NOTE: Slides are the author's property. They may contain unpublished or preliminary information and should only be used while viewing the talk.
TBD
Participants
TBD
UGMS Sites
Download a preliminary site list with Vs30 and basin depth information. Note that CyberShake applies a minimum Vs floor of 500 m/s.
Data
We have extracted timeseries data for the following 4 events:
- Southern San Andreas, nucleating near Bombay Beach (33.3772, -115.74, 4.1514 km deep): source 59, rupture 3, rupture variation 0.
Plots available here. - Southern San Andreas, nucleating near the Carrizo Plain (35.2809, -119.8182, 12.3263 km deep): source 59, rupture 3, rupture variation 296.
Plots available here. - Southern San Andreas, nucleating near the Cajon Pass (34.3123, -117.5051, 20.3019 km deep): source 59, rupture 3, rupture variation 144.
Plots available here. - Puente Hills (34.0811, -118.0461, 12.4803 km deep): source 242, rupture 26, rupture variation 31.
Plots available here.
