Published July 2014 | Version Supplemental Material + Published
Journal Article Open

Response of rate-and-state seismogenic faults to harmonic shear-stress perturbations

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Laboratoire de Géologie de l'École Normale Supérieure

Abstract

Field and laboratory observations show that seismicity has non-trivial period-dependent response to periodic stress perturbations. In Nepal, seismicity shows significant variations in response to annual monsoon-induced stress variations but not to semidiurnal tidal stresses of the same magnitude. Such period dependence cannot be explained by the Coulomb failure model and spring-slider rate-and-state model (SRM). Here, we study seismicity response to periodic stress perturbations in a 2-D continuum model of a rate-and-state fault (that is, a finite rate-and-state fault). We find that the resulting seismicity indeed exhibits nearly periodic variations. Their amplitude is maximum at a certain period, T_a, and decreases with smaller and larger periods to the SRM predictions, remaining much larger than the SRM predictions for a wide range of periods around T_a. We attribute the higher sensitivity of finite faults to their finite nucleation zones which vary in space and have a different slip-velocity evolution than that of the SRM. At periods T ≫ T_a and T ≪ T_a, the seismicity-rate variations are in phase with the stress-rate and stress variations, respectively, consistent with the SRM, although a gradual phase shift appears as T increases towards T_a. Based on the similarities with the SRM and our simulations, we propose a semi-analytical expression for T_a. Plausible sets of model parameters make T_a equal to 1 yr, potentially explaining Nepal observations and constraining the fault properties. Our finite-fault findings indicate that aσ, where a is a rate-and-state parameter and σ is the effective normal stress, can be severely underestimated based on the SRM.

Additional Information

© The Authors 2014. Published by Oxford University Press on behalf of The Royal Astronomical Society. Accepted 2014 April 14. Received 2014 April 10; in original form 2013 September 20. This project was supported by the Gordon and Betty Moore Foundation, through the Tectonics Observatory, NSF grant EAR #0838495. This is Caltech Tectonic Observatory's contribution number 231 and Caltech Seismolab contribution number 10093.

Attached Files

Published - Geophys._J._Int.-2014-Ader-385-413.pdf

Supplemental Material - supplements_papernadia_thesis.pdf

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Additional details

Identifiers

Eprint ID
49020
Resolver ID
CaltechAUTHORS:20140828-112246557

Funding

Gordon and Betty Moore Foundation
Caltech Tectonics Observatory
NSF
EAR 0838495

Dates

Created
2014-08-28
Created from EPrint's datestamp field
Updated
2021-11-10
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Caltech Tectonics Observatory, Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)
Other Numbering System Name
Caltech Division of Geological and Planetary Sciences
Other Numbering System Identifier
10093