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Published December 10, 2010 | Published
Journal Article Open

Three-dimensional earthquake sequence simulations with evolving temperature and pore pressure due to shear heating: Effect of heterogeneous hydraulic diffusivity

Abstract

A new methodology for three-dimensional (3-D) simulations of earthquake sequences is presented that accounts not only for inertial effects during seismic events but also for shear-induced temperature variations on the fault and the associated evolution of pore fluid pressure. In particular, the methodology allows to capture thermal pressurization (TP) due to frictional heating in a shear zone. One-dimensional (1-D) diffusion of heat and pore fluids in the fault-normal direction is incorporated using a spectral method, which is unconditionally stable, accurate with affordable computational resources, and highly suitable to earthquake sequence calculations that use variable time steps. The approach is used to investigate the effect of heterogeneous hydraulic properties by considering a fault model with two regions of different hydraulic diffusivities and hence different potential for TP. We find that the region of more efficient TP produces larger slip in model-spanning events. The slip deficit in the other region is filled with more frequent smaller events, creating spatiotemporal complexity of large events on the fault. Interestingly, the area of maximum slip in model-spanning events is not associated with the maximum temperature increase because of stronger dynamic weakening in that area. The region of more efficient TP has lower interseismic shear stress, which discourages rupture nucleation there, contrary to what was concluded in prior studies. Seismic events nucleate in the region of less efficient TP where interseismic shear stress is higher. In our model, hypocenters of large events do not occur in areas of large slip or large stress drop.

Additional Information

© 2010 American Geophysical Union. Received 13 June 2010; accepted 27 September 2010; published 10 December 2010. This study was supported by National Science Foundation grant EAR 0548277, U.S. Geological Survey grant 08HQGR0057, and Southern California Earthquake Center (SCEC). SCEC is funded by NSF Cooperative Agreement EAR‐0106924 and USGS Cooperative Agreement 02HQAG0008. This is SCEC contribution 1432. The numerical simulations for this research were performed on Caltech Division of Geological and Planetary Sciences Dell cluster. We thank Toshihiko Shimamoto and Wataru Tanikawa for discussions on their geological observations. We thank Associate Editor Robert Nowack and reviewers Andrea Bizzarri and Takehito Suzuki for detailed comments that improved this paper.

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