Group B, Poster #250, San Andreas Fault System (SAFS)
Loma Prieta Again: Subsurface Geology and the San Andreas Fault, Santa Cruz Mountains, Central California
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Poster Presentation
2022 SCEC Annual Meeting, Poster #250, SCEC Contribution #12084 VIEW PDF
d Thurber (2012), potential-field data collected by the U.S. Geological Survey (USGS) following the earthquake, and seismic refraction and reflection data from the 1991 profile of Catchings et al. (2004). The seismic-velocity model and aftershock relocations of Lin and Thurber (2012) reveal a geometry for the SAF that appears similar to that in the Coachella Valley (although rotated 180 degrees): at Loma Prieta the fault dips steeply near the surface and curves with depth to join the moderately southwest-dipping main rupture below 6-km depth, itself also non-planar. The SAF is a clear seismic-velocity boundary, with higher velocities on the northeast, attributable to Mesozoic accretionary and other rocks, and lower velocities on the southwest, attributable to Cenozoic sedimentary and volcanic rocks of the La Honda block. Rocks of the La Honda block have been offset right-laterally hundreds of kilometers from similar rocks in the southern San Joaquin Valley and vicinity, providing evidence that the curved northeast fault boundary of this block is the plate boundary. Thus, we interpret that the Loma Prieta earthquake occurred on the SAF and not on a secondary fault.
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