Theoretical studies have shown that the issue of rupture modes has important implications for fault constitutive laws, stress conditions on faults, energy partition and heat generation during earthquakes, scaling laws, and spatiotemporal complexity of fault slip. Early theoretical models treated earthquakes as crack-like ruptures, but seismic inversions indicate that earthquake ruptures may propagate in a self-healing pulse-like mode. A number of explanations for the existence of slip pulses have been proposed and continue to be vigorously debated. This study presents experimental observations of spontaneous pulse-like ruptures in a homogeneous linear-elastic setting that mimics crustal earthquakes; reveals how different rupture modes are s...
We study in-plane ruptures on a bimaterial fault governed by a velocity-weakening friction with a re...
An edited version of this paper was published by AGU. Copyright (2010) American Geophysical Union.He...
Low-velocity fault zones (LVFZs) are found in most mature faults. They are usually 100–400 m wide an...
Seismic inversions show that earthquake risetimes may be much shorter than the overall rupture durat...
Seismic inversions show that earthquake risetimes may be much shorter than the overall rupture durat...
Destructive large earthquakes occur as dynamic frictional ruptures along pre-existing interfaces (or...
[1] Seismic inversions show that earthquake risetimes may be much shorter than the overall rupture d...
Although kinematic earthquake source inversions show dominantly pulse-like subshear rupture behavior...
Although kinematic earthquake source inversions show dominantly pulse-like subshear rupture behavior...
Faults are usually surrounded by damaged zones of lower elastic moduli and seismic wave velocities t...
Damage zones are ubiquitous components of faults that may affect earthquake rupture. Simulations sho...
Damage zones are ubiquitous components of faults that may affect earthquake rupture. Simulations sho...
Faults are usually surrounded by damaged zones of lower elastic moduli and seismic wave velocities t...
We study in-plane ruptures on a bimaterial fault governed by a velocity-weakening friction with a re...
Low-velocity fault zones (LVFZs) are found in most mature faults. They are usually 100–400 m wide an...
We study in-plane ruptures on a bimaterial fault governed by a velocity-weakening friction with a re...
An edited version of this paper was published by AGU. Copyright (2010) American Geophysical Union.He...
Low-velocity fault zones (LVFZs) are found in most mature faults. They are usually 100–400 m wide an...
Seismic inversions show that earthquake risetimes may be much shorter than the overall rupture durat...
Seismic inversions show that earthquake risetimes may be much shorter than the overall rupture durat...
Destructive large earthquakes occur as dynamic frictional ruptures along pre-existing interfaces (or...
[1] Seismic inversions show that earthquake risetimes may be much shorter than the overall rupture d...
Although kinematic earthquake source inversions show dominantly pulse-like subshear rupture behavior...
Although kinematic earthquake source inversions show dominantly pulse-like subshear rupture behavior...
Faults are usually surrounded by damaged zones of lower elastic moduli and seismic wave velocities t...
Damage zones are ubiquitous components of faults that may affect earthquake rupture. Simulations sho...
Damage zones are ubiquitous components of faults that may affect earthquake rupture. Simulations sho...
Faults are usually surrounded by damaged zones of lower elastic moduli and seismic wave velocities t...
We study in-plane ruptures on a bimaterial fault governed by a velocity-weakening friction with a re...
Low-velocity fault zones (LVFZs) are found in most mature faults. They are usually 100–400 m wide an...
We study in-plane ruptures on a bimaterial fault governed by a velocity-weakening friction with a re...
An edited version of this paper was published by AGU. Copyright (2010) American Geophysical Union.He...
Low-velocity fault zones (LVFZs) are found in most mature faults. They are usually 100–400 m wide an...