Long-Term Fault Slip in Models With Coseismic Weakening: Depth Extent and Spatio-Temporal Complexity of Earthquake Ruptures
Abstract:
Using 3D rate-and-state fault models with temperature and pore pressure evolution, we study the effect of depth-dependent permeability and shear-zone width on long-term fault slip. Competition between the two properties determines the depth dependence of co-seismic weakening due to TP, since permeability decreases with depth (due to higher compression), promoting TP, while the shear-zone width likely increases below certain depth (due to increasingly inelastic bulk properties), lowering the co-seismic temperature increase and suppressing TP.
We find that, indeed, large ruptures can penetrate below the traditionally defined SL, into the “stable” fault regions, due to TP. When they do, microseismicity patterns at the bottom of the SL change, potentially allowing for identification of such penetration in recent events. The behavior of large ruptures, including their depth extent, varies along strike, even though the fault properties are uniform along strike. This is because co-seismic weakening is strongly dependent on the local rupture properties (slip rate and slip), setting up a strong feedback loop between the weakening and rupture response. The non-uniform slip during one event leads to spatio-temporal complexity in subsequent events, including large variations of depth extent with time. Our current efforts are directed towards quantifying these effects, including the relation between rupture slip, depth, and length as well as their variability.
