Non-SAF type focal mechanisms adjacent to the SAF, Mojave Segment: Implications for Blind Thrust Beneath the San Gabriel Mountains, Southern California
- Creators
- Huang, Weishi
- Silver, Leon T.
- Kanamori, Hiroo
- Other:
- Chen, Zhangli
Abstract
Focal mechanisms of earthquakes with 2.5 ≤ M ≤ 4.1 from 1978 to 1990 were analyzed within a 15 km-wide belt of the San Andreas fault (SAF) zone, in the Mojave segment, southern California. Of the 29 events, 41% are strike-slip, 28% oblique--slip, 24% thrust, and 7% are normal fault types. Most of the thrust events are located in the central section of the studied zone, where the fault geometry is relatively simple. In contrast, most of the strike-slip events arc at the intersection between the SAF and the San Jacinto fault. Both stress tensor inverted from slip vectors and strain tensor calculated from earthquake moment tensors produce similar directions of maximum principal compressional axes that arc oriented in the direction between 351° and 5°, which is at an angle of about 60° to the strike of the SAF. These non-SAF type faulting events obviously can not be explained by simple shear motion on the SAF. Instead, they accrued on the structures that were activated in response to the regional N compression at the latitude of the Transverse Ranges. For the thrust events, we interpret that a back thrust (northward thrust) exists beneath the northern side of the San Gabriel Mountains. This back thrust is located at the depth of 8-13 km, within or beneath the Pelona schist. It is apparently associated with aseismic slip and uplifts the San Gabriel Mountains on the northern side.
Additional Information
© 1993 Beijing Seismological Press. We thank Ding Guoyu for his enthusiastic discussions and for his help to make this paper published. Discussions with Gao Weiming, Ma Zonjing, and Paul Tapponnier during this meeting arc also appreciated. We thank Steve Bryant for his help in checking the first motion data, Clarence Allen and Egill Hauksson for helpful discussions. This work is supported by the U.S. Geol. Survey Grant 14-08-0001-G1774. Contribution Number 5239, Seismological Laboratory, Division of Geological and Planetary Sciences, California Institute of Technology.Additional details
- Eprint ID
- 51544
- Resolver ID
- CaltechAUTHORS:20141111-080640739
- USGS
- 14-08-0001-G1774
- Created
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2014-11-11Created from EPrint's datestamp field
- Updated
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2019-11-21Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences
- Series Name
- IASPEI Publication Series for the IDNDR
- Series Volume or Issue Number
- 3
- Other Numbering System Name
- Caltech Division of Geological and Planetary Sciences
- Other Numbering System Identifier
- 5239