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Time-Dependent Seismology

Anderson, Don L. and Whitcomb, J. H. (1975) Time-Dependent Seismology. Journal of Geophysical Research, 80 (11). pp. 1497-1503. ISSN 0148-0227. http://resolver.caltech.edu/CaltechAUTHORS:20150220-070523447

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Abstract

The time variation of crustal velocities in tectonic regions is most reasonably attributed to stress induced variations in crack porosity. The decrease in V_p/V_s before earthquakes is due primarily to a large decrease in V_p. This supports the Nur dilatancy hypothesis but not the effective stress hypothesis. New data from the San Fernando region verify the V_p drop, show that this drop cannot be entirely due to source depth effects, and give strong support to the explanation of material property, or path effect, rather than source effect variations. Calculations show that the crack-widening model works even for mid crustal depths in saturated rock. Narrow cracks of low aspect ratio are required to satisfy the velocity and uplift constraints. The recovery of velocity prior to fracture can be due to fluid flow or crack closure. The t ∼ L^2 relation does not require diffusion. Diffusion of groundwater or crack closure leads to increased pore pressure and rock weakening. Observations of gravity, conductivity, and crustal distortions along with velocities should narrow the choice of models. The crust in regions of thrust tectonics is probably always dilatant to some degree. The aftershock region is smaller than the anomalous velocity region, which in turn must be smaller than the dilatant region. A simple relationship is derived for the relative sizes of the anomalous and aftershock regions.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/JB080i011p01497DOIArticle
http://onlinelibrary.wiley.com/doi/10.1029/JB080i011p01497/abstractPublisherArticle
Additional Information:© 1975 by the American Geophysical Union. Received May 10, 1974; revised November 8, 1974; accepted November 19, 1974. Article first published online: 20 Sep 2012. This research was supported by the National Science Foundation grant NSF GA 29920 and grants from the Jet Propulsion Laboratory and Standard Oil Company of California. We appreciate conversations with R. O'Connell and B. Budiansky and a preprint kindly provided by B. Brady in advance of publication. Contribution 2363, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California.
Funders:
Funding AgencyGrant Number
NSFGA 29920
JPLUNSPECIFIED
Standard Oil Company of CaliforniaUNSPECIFIED
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Caltech Division of Geological and Planetary Sciences2363
Record Number:CaltechAUTHORS:20150220-070523447
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150220-070523447
Official Citation:Anderson, D. L., and J. H. Whitcomb (1975), Time-dependent seismology, J. Geophys. Res., 80(11), 1497–1503, doi:10.1029/JB080i011p01497.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55037
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:20 Feb 2015 15:37
Last Modified:13 Feb 2019 18:06

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