The Fine-Scale Structure of Long Beach, California, and Its Impact on Ground Motion Acceleration
- Creators
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Castellanos, Jorge C.
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Clayton, Robert W.
Abstract
The metropolitan Los Angeles region represents a zone of high-seismic risk due to its proximity to several fault systems, including the San Andreas fault. Adding to this problem is the fact that Los Angeles and its surrounding cities are built on top of soft sediments that tend to trap and amplify seismic waves generated by earthquakes. In this study, we use three dense petroleum industry surveys deployed in a 16 × 16-km area at Long Beach, California, to produce a high-resolution model of the top kilometer of the crust and investigate the influence of its structural variations on the amplification of seismic waves. Our velocity estimates reveal substantial lateral contrasts and correlate remarkably well with the geological background of the area, illuminating features such as the Newport-Inglewood fault, the Silverado aquifer, and the San Gabriel river. We then use computational modeling to show that the presence of these small-scale structures have a clear impact on the intensity of the expected shaking, and can cause ground-motion motion acceleration to change by several factors over a subkilometer horizontal scale. These results shed light onto the scale of variations that can be expected in this type of tectonic settings and highlight the importance of resolution in modern-day seismic hazard estimates.
Additional Information
© 2021. American Geophysical Union. Issue Online: 13 December 2021; Version of Record online: 13 December 2021; Accepted manuscript online: 17 November 2021; Manuscript accepted: 05 November 2021; Manuscript revised: 01 October 2021; Manuscript received: 21 May 2021. The authors gratefully acknowledge NodalSeismic and Signal Hill Petroleum for allowing us to use the Long Beach and Extended Long Beach data, and LA seismic for the use of the Seal Beach data. Permission form these organizations is required to access the data. They thank Dan Hollis and Eric Campbell for facilitating the use of the seismic data. They extend our acknowledgement to Dan Gish and Steve Boljen for providing us with the migrated seismic sections of the Seal Beach survey. They also thank Michael Afanasiev and the Mondaic team for their help in setting up the numeric simulations. They are grateful to Zhe Jia for providing us with the ambient noise cross-correlations between the nodal instruments and the SCSN seismic station, and to Bruce Worden for providing us with the Vs30 measurements. They gratefully thank Nori Nakata, Hongjian Fang, and an anonymous reviewer for their careful and constructive suggestions. This project was partially supported by NSF/EAER-1520081. Data Availability Statement: The 3-D shear wave velocity model that is presented in this work can be downloaded from: https://doi.org/10.22002/D1.1970.Attached Files
Published - 2021JB022462.pdf
Submitted - essoar10507964.2.pdf
Supplemental Material - 2021jb022462-sup-0001-supporting_information_si-s01.pdf
Supplemental Material - 2021jb022462-sup-0002-movie_si-s01.mp4
Supplemental Material - 2021jb022462-sup-0003-movie_si-s02.mp4
Supplemental Material - 2021jb022462-sup-0004-movie_si-s03.mp4
Supplemental Material - 2021jb022462-sup-0005-movie_si-s04.mp4
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Additional details
- Eprint ID
- 111377
- Resolver ID
- CaltechAUTHORS:20211012-211827814
- NSF
- EAR-1520081
- Created
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2021-10-13Created from EPrint's datestamp field
- Updated
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2023-10-04Created from EPrint's last_modified field
- Caltech groups
- Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)