Difference between revisions of "CyberShake Study 22.12"
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− | | [[File:WNGC_run4293_spectral.png|thumb|400px|Spectral plot for WNGC from Study 15.12, target of 0.3676g @ 3 sec]] | + | | [[File:WNGC_run4293_spectral.png|thumb|400px|Spectral plot for WNGC from Study 15.12, target of 0.3676g @ 3 sec. Mean is in red.]] |
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+ | It appears that the 706 rupture variations in the above plot are producing higher-than-average ground motions. Below is a similar plot, but which includes all rupture variations, and the overall mean (in orange). | ||
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+ | | [[File:WNGC_run4293_full_spectral.png|thumb|400px|Spectral plot for WNGC from Study 15.12, all variations.]] | ||
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Revision as of 19:21, 19 September 2022
CyberShake Study 22.10 is a proposed study in Southern California which will include deterministic low-frequency (0-1 Hz) and stochastic high-frequency (1-50 Hz) simulations. We will use the Graves & Pitarka (2019) rupture generator and the high frequency modules from the SCEC Broadband Platform v22.4.
Contents
- 1 Status
- 2 Data Products
- 3 Science Goals
- 4 Technical Goals
- 5 Sites
- 6 Velocity Model
- 7 High-frequency codes
- 8 Spectral Content around 1 Hz
- 9 Verification
- 10 Updates and Enhancements
- 11 Output Data Products
- 12 Computational and Data Estimates
- 13 Lessons Learned
- 14 Stress Test
- 15 Performance Metrics
- 16 Production Checklist
- 17 Presentations, Posters, and Papers
Status
This study is in the planning phase. We estimate calculations will begin in October 2022.
Data Products
Science Goals
Technical Goals
Sites
Velocity Model
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 hfsims_cfg.py 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.
It appears that the 706 rupture variations in the above plot are producing higher-than-average ground motions. Below is a similar plot, but which includes all rupture variations, and the overall mean (in orange).
Verification
Updates and Enhancements
Output Data Products
Computational and Data Estimates
Lessons Learned
Stress Test
Performance Metrics
Production Checklist
Science to-dos
- Perform validation for Northridge, Chino Hills, Whittier, Landers, Hector Mine, and North Palm Springs
- For each validation event, calculate BBP results, CS results, and CS results with BBP Vs30 values
- 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
Technical to-dos
Integrate refactoring of BBP codes into latest BBP releaseSwitch to using github repo version of CyberShake on SummitUpdate 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