T108 Woollard Session: Interdisciplinary Insights into Fault Zone Properties and Faulting Processes (Posters)
Monday, 23 September 2024
8:00 AM - 5:30 PM
Hall D
QUANTIFYING THE EFFECTS OF ABSOLUTE FRICTION AND SYMMETRY ON THRUST FAULT RUPTURE
Paper number: T108-2
Program: Technical Sessions
Time: 8:00 AM – 5:30 PM
Authors
-
David OglesbyUniversity of California, Riverside, Riverside, CA
Abstract
Our approach uses dynamic finite element modeling to simulate rupture propagation and slip during a thrust earthquake. We model a 2-dimensional 40 km-long, 15º dipping thrust fault within a homogenous solid using the finite element code FaultMod developed by Michael Barall. For each condition of absolute friction, three models are conducted: (1) where the upper fault tip terminates at the free surface; (2) where the upper fault tip is buried 9 km; and (3) where the upper fault tip is buried 120 km. For the latter model, seismic radiation is unable to reflect off the free surface to the fault before slip ceases. For the other two models, seismic radiation from the free surface can interact with the fault as rupture propagates, thereby causing changes in the normal stress and influencing slip.
Preliminary results for a purely symmetric fault in a whole-space both confirm and demonstrate that different frictional and stress parameterizations produce identical final slip results in a symmetric configuration. For models that approach the free surface, where the free surface boundary condition is apparent, we find that the evolution of fault rupture and slip do indeed depend on the absolute level of friction. We believe our findings will provide valuable insight in investigating real-world thrust earthquakes, specifically demonstrating the relationship between friction and geometrical symmetry to the temporal evolution of slip and stress during an earthquake.
Geological Society of America Abstracts with Programs. Vol. 56, No. 5
doi: 10.1130/abs/2024AM-403530
© Copyright 2024 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.