Comparison between crustal density and velocity variations in southern California
- Creators
- Langenheim, V. E.
-
Hauksson, Egill
Abstract
We predict gravity from a three-dimensional V_p model of the upper crust and compare it to the observed isostatic residual gravity field. In general this comparison shows that the isostatic residual gravity field reflects the density variations in the upper to middle crust. Both data sets show similar density variations for the upper crust in areas such as the Peninsular Ranges and the Los Angeles basin. Both show similar variations across major faults, such as the San Andreas and Garlock faults in the Mojave Desert. The difference between the two data sets in regions such as the Salton Trough, the Eastern California Shear Zone, and the eastern Ventura basin (where depth to Moho is <30 km), however, suggests high-density middle to lower crust beneath these regions. Hence the joint interpretation of these data sets improves the depth constraints of crustal density variations.
Additional Information
© 2001 by the American Geophysical Union. Received May 3, 2001; accepted June 18, 2001. Research was supported in part by U.S.G.S. grant 01HGR0038, and from the Southern California Earthquake Center to E. Hauksson (SCEC contribution 579). Contribution 8760, Div. of Geol. and Planetary Sciences, Caltech, Pasadena. We thank two anonymous reviewers, T.M. Brocher and R.J. Blakely, and comments by R.W. Simpson, R.C. Jachens, and T.G. Hilde.Attached Files
Published - grl14897.pdf
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Additional details
- Eprint ID
- 36963
- Resolver ID
- CaltechAUTHORS:20130215-134619909
- USGS
- 01HGR0038
- Southern California Earthquake Center (SCEC)
- Created
-
2013-02-15Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)
- Other Numbering System Name
- Caltech Division of Geological and Planetary Sciences
- Other Numbering System Identifier
- 8760