Transient gravity perturbations induced by earthquake rupture
Abstract
The static and transient deformations produced by earthquakes cause density perturbations which, in turn, generate immediate, long-range perturbations of the Earth's gravity field. Here, an analytical solution is derived for gravity perturbations produced by a point double-couple source in homogeneous, infinite, non-self-gravitating elastic media. The solution features transient gravity perturbations that occur at any distance from the source between the rupture onset time and the arrival time of seismic P waves, which are of potential interest for real-time earthquake source studies and early warning. An analytical solution for such prompt gravity perturbations is presented in compact form. We show that it approximates adequately the prompt gravity perturbations generated by strike-slip and dip-slip finite fault ruptures in a half-space obtained by numerical simulations based on the spectral element method. Based on the analytical solution, we estimate that the observability of prompt gravity perturbations within 10 s after rupture onset by current instruments is severely challenged by the background microseism noise but may be achieved by high-precision gravity strainmeters currently under development. Our analytical results facilitate parametric studies of the expected prompt gravity signals that could be recorded by gravity strainmeters.
Additional Information
© 2015 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society. Accepted 2015 February 20. Received 2015 February 11; in original form 2014 October 22. We thank Eric Clévédé for discussions during the initial phase of this study and Mauricio Fuentes for assistance with verification and simplification of analytical derivations. This work was supported by NSF Grants PHY 0855313 and PHY 1205512 to UF. BFW acknowledges sabbatical support from the Université Paris Diderot and the CNRS through the APC, where part of this work was carried out. JPA acknowledges support by a grant from the Gordon and Betty Moore Foundation to Caltech. We acknowledge the financial support from the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02) and the financial support of the Agence Nationale de la Recherche through the grant ANR-14-CE03-0014-01. SPECFEM3D is available at http://www.geodynamics.org/cig/software/specfem3d.Attached Files
Published - Geophys._J._Int.-2015-Harms-1416-25.pdf
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Additional details
- Eprint ID
- 58337
- Resolver ID
- CaltechAUTHORS:20150618-084429927
- NSF
- PHY 0855313
- NSF
- PHY 1205512
- Université Paris Diderot
- Centre National de la Recherche Scientifique (CNRS)
- Gordon and Betty Moore Foundation
- Sorbonne Paris Cité
- ANR-10-LABX-0023
- Sorbonne Paris Cité
- ANR-11-IDEX-0005-02
- Agence Nationale de la Recherche (ANR)
- ANR-14-CE03-0014-01
- Created
-
2015-06-19Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Seismological Laboratory