A mechanism for preseismic steady rupture fronts observed in laboratory experiments
- Creators
- Kaneko, Y.
-
Ampuero, J.-P.
Abstract
It has been shown that the onset of frictional instability is characterized by a transition from stable, quasi-static rupture growth to unstable, inertially-controlled high-speed rupture. In particular, slow rupture fronts propagating at a steady speed V_(slow) of the order of 5% of the S-wave speed have been observed prior to the onset of dynamic rupture in recent fault-friction laboratory experiments. However, the precise mechanism governing this V_(slow) stage is unknown. Here we reproduce this phenomenon in numerical simulations of earthquake sequences that incorporate laboratory-derived rate-and-state friction laws. Our simulations show that the V_(slow) stage originates from a stress concentration inherited from the coalescence of interseismic slow creep fronts. Its occurrence is limited to a narrow range of the parameter space but is found in simulations with two commonly-used state-variable evolution laws in the rate-and-state formulation. The sensitivity of the speed V_(slow) to the model parameters suggests that the propagation speed V_(slow) reported in laboratory experiments may also be sensitive to parameters of friction and stress conditions. Our results imply that time and space dimensions associated with the propagation of V_(slow) on natural faults can be as much as a few seconds and several hundred meters, respectively. Hence the detection of such preseismic signals may be possible with near-field high-resolution observations.
Additional Information
© 2011 by the American Geophysical Union. Received 10 October 2011; accepted 11 October 2011; published 10 November 2011. The authors thank Stefan Nielsen for sharing the results of his laboratory experiments. The reviews by Maria Elina Belardinelli and an anonymous reviewer helped us improve the manuscript. This study was supported by NSF (grant EAR‐1015698) and SCEC (funded by NSF Cooperative Agreement EAR‐0106924 and USGS Cooperative Agreement 02HQAG0008). This is SCEC contribution number 1511. [26] The Editor thanks Maria Elina Belardinelli and an anonymous reviewer for their assistance in evaluating this paper.Attached Files
Published - Kaneko2011p16467Geophys_Res_Lett.pdf
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Additional details
- Eprint ID
- 28456
- Resolver ID
- CaltechAUTHORS:20111213-144536891
- NSF
- EAR-1015698
- NSF
- EAR‐0106924
- USGS
- 02HQAG0008
- Created
-
2011-12-14Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Seismological Laboratory
- Other Numbering System Name
- Southern California Earthquake Center (SCEC)
- Other Numbering System Identifier
- 1511