Quasi-dynamic versus fully dynamic simulations of earthquakes and aseismic slip with and without enhanced coseismic weakening
Abstract
Physics-based numerical simulations of earthquakes and slow slip, coupled with field observations and laboratory experiments, can, in principle, be used to determine fault properties and potential fault behaviors. Because of the computational cost of simulating inertial wave-mediated effects, their representation is often simplified. The quasi-dynamic (QD) approach approximately accounts for inertial effects through a radiation damping term. We compare QD and fully dynamic (FD) simulations by exploring the long-term behavior of rate-and-state fault models with and without additional weakening during seismic slip. The models incorporate a velocity-strengthening (VS) patch in a velocity-weakening (VW) zone, to consider rupture interaction with a slip-inhibiting heterogeneity. Without additional weakening, the QD and FD approaches generate qualitatively similar slip patterns with quantitative differences, such as slower slip velocities and rupture speeds during earthquakes and more propensity for rupture arrest at the VS patch in the QD cases. Simulations with additional coseismic weakening produce qualitatively different patterns of earthquakes, with near-periodic pulse-like events in the FD simulations and much larger crack-like events accompanied by smaller events in the QD simulations. This is because the FD simulations with additional weakening allow earthquake rupture to propagate at a much lower level of prestress than the QD simulations. The resulting much larger ruptures in the QD simulations are more likely to propagate through the VS patch, unlike for the cases with no additional weakening. Overall, the QD approach should be used with caution, as the QD simulation results could drastically differ from the true response of the physical model considered.
Additional Information
© 2014 American Geophysical Union. Received 28 August 2013; Accepted 22 January 2014; Accepted article online 28 January 2014; Published online 20 March 2014. This study was supported by the National Science Foundation through grant EAR 1142183, the Gordon and Betty Moore Foundation through grant GBMF 423.01 to the Caltech Tectonics Observatory, and the Keck Institute for Spaces Studies at Caltech. This is Tectonics Observatory contribution 255. The numerical simulations for this research were performed on Caltech Division of Geological and Planetary Sciences Dell cluster. We thank reviewers Steve Day and Ruth Harris for insightful detailed comments that helped us improve the manuscript.Attached Files
Published - jgrb50520.pdf
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Additional details
- Eprint ID
- 46810
- Resolver ID
- CaltechAUTHORS:20140703-104019674
- NSF
- EAR 1142183
- Gordon and Betty Moore Foundation
- GBMF 423.01
- Keck Institute for Space Studies (KISS)
- Created
-
2014-07-07Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Keck Institute for Space Studies, Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)
- Other Numbering System Name
- Tectonics Observatory
- Other Numbering System Identifier
- 255