Group B, Poster #086, Tectonic Geodesy
Estimating the surface creep rate of the central San Andreas fault from a 3D surface velocity field derived from UAVSAR and Sentinel-1 data
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Poster Presentation
2024 SCEC Annual Meeting, Poster #086, SCEC Contribution #13658 VIEW PDF
ends across the whole seismogenic layer of the crust, meaning the whole fault segment is exhibiting stable sliding. To better visualize and estimate the surface creep rates of the central SAF, we jointly used UAVSAR and Sentinel-1 SAR images to build the secular 3D surface velocity field. We then projected the East-West and North-South components into fault-parallel and fault-perpendicular directions and made 110 cross-fault profiles through the fault-parallel velocity field to estimate the distribution of surface creep rates along strike. The creep rates at the southern end (north of Parkfield and south of Bitterwater) exceeded 2 cm/yr with some parts reaching close to 3 cm/yr. At the northern end of the central SAF, creep appears to be partitioned between the SAF and the Calaveras fault and thus the SAF creep rates drop down to ~1cm/yr. These findings agree with previous investigations, and given the high spatial resolution that InSAR data offers, our results can be used as the starting step for identifying how creep varies temporally and/or spatially in order to understand its decadal kinematic evolution.
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