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Annual Meeting - SCEC.org

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Poster Abstracts<br />

San Andreas fault system, and an earthquake early warning can be issued. We show results from the southern Californian<br />

CRTN sites during the 2010 Mw 7.2 El Mayor-Cucapah earthquake. The data collected showed significant ground motions in<br />

the Imperial Valley a few seconds after the initial earthquake and for a few minutes, the movement reverberated across all of<br />

southern California (Bock et al., 2011). The SOPAC group is working on rapid determination of earthquake location,<br />

magnitude and fault plane using the site displacements computed by the network adjustment (Crowell et al., 2009; Melgar et<br />

al., 2011).<br />

MECHANICS OF STRESS TRANSFER FROM PLATE MOTION TO PLATE BOUNDARY FAULTS: DYNAMIC<br />

MODELS OF EARTHQUAKE CYCLES ON A STRIKE-SLIP FAULT (B-146)<br />

C.S. Takeuchi and Y. Fialko<br />

Existing models of interseismic deformation are predominantly kinematic: loading is applied by prescribing slip on<br />

dislocations, either at a constant rate below the seismogenic layer (the Savage-Burford model) or quasi-periodically in the<br />

seismogenic layer on top of a viscoelastic substrate (the Elsasser model). These loading mechanisms are not physically<br />

consistent. In particular, kinematic viscoelastic cycle models produce absolute stresses on the seismogenic fault that are<br />

opposite to the sense of tectonic loading. We consider dynamic (stress-controlled) models of strike-slip faults that are driven<br />

by far-field tractions due to relative plate motion. We use antiplane strain finite element models to simulate quasi-periodic<br />

earthquakes on a fault in a brittle crust underlain by a viscoelastic medium. Each model is driven by far-field plate motion at a<br />

rate of 4 cm/yr, similar to the San Andreas Fault (SAF) in California. Slip occurs when the shear stress on the fault exceeds a<br />

prescribed threshold. We analyze stresses, strain rates, and surface deformation for models assuming various rheologies of a<br />

ductile substrate, including a) linear Maxwell rheology, b) power law temperature dependent rheology assuming a given<br />

linear geotherm, and c) power law temperature dependent rheology with thermo-mechanical coupling. The latter class of<br />

models gives rise to a permanent localized shear zone due to the interaction of viscous dissipation and heat conduction. An<br />

initial temperature perturbation is generated via a kinematically-driven thermal “maturation” of the fault at a constant slip<br />

rate over “geological” (millions of years) time scales. Strain localization in the power law viscoelastic medium due to thermomechanical<br />

coupling is used as a proxy for all strain-weakening mechanisms (including e.g. grain-size reduction). Simulations<br />

are performed for “dry” and “wet” rheological endmembers for the viscoelastic substrate. We compare the predicted surface<br />

velocities and strain rates to available observations from the SAF. We find that a dry temperature-dependent power law<br />

rheology best reproduces time-dependent surface deformation and generates reasonable deviatoric stresses in the crust and<br />

upper mantle.<br />

STATIC DISPLACEMENTS COMPUTED FROM SEISMIC WAVEFIELD SIMULATIONS: VALIDATION<br />

TESTS FOR HOMOGENEOUS AND 1D STRUCTURE (A-061)<br />

C. Tape, J.P. Loveless, and B.J. Meade<br />

Earthquake 240 240 c 240 y 240 c 240 l 240 e 240 240 p 240 r 240 o 240 c 240 e 240 s 240 s 240 240 i 240 n 240<br />

240 s 240 o 240 u 240 t 240 h 240 e 240 r 240 n 240 240 C 240 a 240 l 240 i 240 f 240 o 240 r 240 n 240 i 240 a 240 240 a 240 r 240 e 240<br />

240 c 240 o 240 m 240 m 240 o 240 n 240 l 240 y 240 240 i 240 n 240 f 240 e 240 r 240 r 240 e 240 d 240 240 f 240 r 240 o 240 m 240<br />

240 m 240 o 240 d 240 e 240 l 240 s 240 240 o 240 f 240 240 g 240 e 240 o 240 d 240 e 240 t 240 i 240 c 240 240 d 240 a 240 t 240 a 240<br />

240 a 240 s 240 s 240 u 240 m 240 i 240 n 240 g 240 240 t 240 h 240 a 240 t 240 240 t 240 h 240 e 240 240 u 240 p 240 p 240 e 240 r 240<br />

240c 240r 240u 240s 240t 240 240c 240a 240n240 240b 240e 240 240t 240r 240e240a 240t 240e 240d 240 240a 240s 240 240a 240<br />

240s240i240m240p240l240e240 240h240o240m240o240g240e240n240e240o240u240s240 240e240l240a240s240t240i240c240<br />

240h240a240l 240f 240s 240p 240a240c240e 240. 240 240H 240o 240w 240e 240v 240e240r 240,240 240i 240t240 240i240s 240<br />

240 w 240 e 240 l 240 l 240 240 k 240 n 240 o 240w 240n 240 240 t 240 h 240 a 240 t 240 240 m 240 a 240 t 240 e 240 r 240 i 240a 240 l 240<br />

240p240r240o240p240e240r240t240i240e240s240 240(240f240o240r240 240e240x240a240m240p240l240e240,240 240V240s240<br />

240o240r240 240V240p240)240 240v240a240r240y240 240b240y240 240m240o240r240e240 240t240h240a240n240 240a240n240<br />

240 o 240 r 240 d 240e 240 r 240 240 o 240 f 240 240 m 240 a 240 g 240n 240 i 240 t 240 u 240 d 240e 240 , 240 240 f 240 r 240 o 240 m 240<br />

240 l 240 o 240 w 240 240 w 240 a 240 v 240 e 240 240 s 240 p 240 e 240 e 240 d 240 s 240 240 i 240 n 240<br />

240u240n240c240o240n240s240o240l240i240d240a240t240e240d240 240s240e240d240i240m240e240n240t240s240 240t240o240<br />

240 h 240 i 240 g 240 h 240 240 w 240 a 240 v 240 e 240 240 s 240 p 240 e 240 e 240 d 240 s 240 240 i 240 n 240 240 t 240 h 240 e 240<br />

240u240p240p240e240r240m240o240s240t240 240m240a240n240t240l240e240 240b240e240l240o240w240 240t240h240e240<br />

240 M 240o 240 h 240 o 240. 240 240T 240h 240i 240s 240 240 r 240 a 240 n 240g 240e 240 240 o 240 f 240 240 w 240a 240 v 240e 240<br />

240 s 240 p 240 e 240 e 240 d 240 s 240 240 i 240 s 240 240 p 240 r 240 e 240 s 240 e 240 n 240 t 240 240 w 240 i 240 t 240 h 240 i 240 n 240<br />

240c240r240u240s240t240a240l240 240m240o240d240e240l240s240 240i240n240 240s240o240u240t240h240e240r240n240<br />

240 | Southern California Earthquake Center

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