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  3. Data Release for the 2018 U.S. Geological Survey–California Geological Survey Fault-Imaging Surveys Across the Hollywood and Santa Monica Faults, Los Angeles County, California

Data Release for the 2018 U.S. Geological Survey–California Geological Survey Fault-Imaging Surveys Across the Hollywood and Santa Monica Faults, Los Angeles County, California

Dates

Publication Date
Start Date
2018-05-23
End Date
2018-06-06

Citation

Goldman, M.R., Catchings, R.D., Chan, J.H., Sickler, R.R., Criley, C.C., Hernandez, J.L., and Olson, B., 2020, Data Release for the 2018 U.S. Geological Survey–California Geological Survey Fault-Imaging Surveys Across the Hollywood and Santa Monica Faults, Los Angeles County, California: U.S. Geological Survey data release, https://doi.org/10.5066/P9ENA8D4.

Summary

We acquired multiple types of controlled-source seismic data across the Hollywood Fault in Hollywood, Calif., and the Santa Monica Fault in Beverly Hills, Calif., in May and June of 2018. We acquired two separate profiles across the Hollywood Fault, and from those data, we can evaluate multiple seismic datasets, including guided-wave data, tomographic Vp data, and tomographic Vs data. From the datasets, we can calculate multiple seismic models, including Vp/Vs and Poisson's ratio models derived from tomographic Vp and Vs data, Rayleigh-wave-based Vs models, Love-wave-based Vs models, Vp/Vs and Poisson's ratio models (derived from combinations of tomographic-based Vp and surface-wave-based Vs models), P-wave reflection images, and S-wave [...]

Contacts

Point of Contact :
Mark R Goldman
Originator :
Mark R Goldman, Rufus D Catchings, Joanne H Chan, Robert R Sickler, Coyn J Criley, Janice L Hernandez, Brian Olson
Metadata Contact :
Mark R Goldman
Publisher :
U.S. Geological Survey
Distributor :
U.S. Geological Survey - ScienceBase
SDC Data Owner :
Earthquake Hazards Program
USGS Mission Area :
Natural Hazards

Attached Files

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hollywood_18.xml
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hollywood_18_as_10.tar 810.39 MB application/x-tar
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hollywood_18_gw_1_C.tar 899.84 MB application/x-tar
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hollywood_18_gw_1_H.tar 206.82 MB application/x-tar
hollywood_18_gw_1_F2.tar 798.88 MB application/x-tar
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hollywood_18_gw_2_H.tar 55.11 MB application/x-tar
hollywood_18_gw_2_D.tar 70.19 MB application/x-tar
hollywood_18_gw_2_C.tar 180.89 MB application/x-tar
hollywood_18_gw_2_A.tar 209.1 MB application/x-tar
hollywood_18_gw_2_G.tar 302.59 MB application/x-tar
hollywood_18_gw_2_F.tar 606.48 MB application/x-tar
hollywood_18_gw_2_B.tar 621.37 MB application/x-tar
hollywood_18_gw_2_E.tar 611.88 MB application/x-tar
hollywood_18.README 14.92 KB text/plain
hollywood_18_as_geophones.csv 5.61 KB text/csv
hollywood_18_gw_deployment.csv 45.86 KB text/csv
hollywood_18_as_shotpoints.csv 5.47 KB text/csv
hollywood_18_as_geophones.csv 5.61 KB text/csv
hollywood_18_as_deployment.csv 19.71 KB text/csv

Purpose

Our goal is to gain a better understanding of the fault structure in the Hollywood and Beverly Hills area.

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DOI https://www.sciencebase.gov/vocab/category/item/identifier doi:10.5066/P9ENA8D4

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