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Finite Difference Simulations of Seismic Scattering: Implications for the Propagation of Short-Period Seismic Waves in the Crust and Models of Crustal Heterogeneity

Frankel, Arthur and Clayton, Robert W. (1986) Finite Difference Simulations of Seismic Scattering: Implications for the Propagation of Short-Period Seismic Waves in the Crust and Models of Crustal Heterogeneity. Journal of Geophysical Research B, 91 (B6). pp. 6465-6489. ISSN 0148-0227. http://resolver.caltech.edu/CaltechAUTHORS:20121016-125457564

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Abstract

Synthetic seismograms produced by the finite difference method are used to study the scattering of elastic and acoustic waves in two-dimensional media with random spatial variations in seismic velocity. The results of this study provide important insights about the propagation of short-period (< 1 s) seismic waves in the earth's crust and place significant constraints on the fluctuation spectrum of crustal heterogeneity on length scales from tens of kilometers to tens of meters. The synthetic seismograms are analyzed to determine the variation in travel times and waveforms across arrays of receivers. The apparent attenuation caused by scattering and the time decay and amplitude of the seismic coda are also quantified with the numerical simulations. Random media with Gaussian and exponential correlation functions are considered, as well as a self-similar medium with equal variations in seismic velocity over a broad range of length scales. These media differ in the spectral falloff of their velocity fluctuations at wavelengths smaller than 2π times the correlation distance a. The synthetic seismograms demonstrate that a random medium with self-similar velocity fluctuations at length scales less than about 50 km (a ≥ 10 km) can explain both travel time anomalies reported for teleseismic arrivals across large-scale seismic arrays (e.g., LASA and NORSAR) and the presence of seismic coda at frequencies of 30 Hz and greater commonly observed in microearthquake waveforms. Media with Gaussian and exponential correlation functions in velocity do not account for both sets of observations for reasonable standard deviations in velocity (≤10%). The scattering attenuation (Q^(−1)) observed in the simulations for Gaussian media is peaked at ka between 1 and 2, where k is the seismic wave number. The observed attenuation in exponential media increases with frequency for ka < 1 and remains about constant for 1 ≤ ka ≤ 5.6. At high frequencies (ka > 5), the self-similar medium is characterized by a scattering Q that is constant with frequency, whereas theory predicts that the apparent Q in an exponential medium is proportional to frequency. These alternative models of crustal heterogeneity can thus be tested by improved measurements of the frequency dependence of crustal Q at frequencies greater than about 1 Hz, assuming that scattering is responsible for most of the attenuation at these frequencies. Measurements of the time decay of the synthetic coda waves clearly show that the single scattering model of coda decay is not appropriate in the presence of moderate amounts of scattering attenuation (scattering Q ≤ 200). In these cases, Q values derived from the coda decay rate using the single scattering theory do not correspond to the transmission Q of the medium. The cross correlation of synthetic waveforms observed for an array of receivers along the free surface is observed to be dependent on the correlation distance of the medium. The self-similar random medium proposed here for the crust produces waveform variations at high frequencies (15–30 Hz) similar to those reported for actual small-scale seismic arrays with apertures of hundreds of meters.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/JB091iB06p06465DOIUNSPECIFIED
http://www.agu.org/pubs/crossref/1986/JB091iB06p06465.shtmlPublisherUNSPECIFIED
Additional Information:© 1986 American Geophysical Union. Received 18 August 1985; revised January 30, 1986; accepted 30 January 1986. John Vidale developed and implemented a substantial portion of the finite difference codes used in this study. W. Menke, P. E. Malin, J. Boatwright, T. C. Hanks, D. J. Andrews, E. Cranswick, and an anonymous reviewer provided useful comments on the manuscript. We particularly thank one of the Associate Editors of JGR for suggestions which significantly improved the paper. The research in this paper was carried out by the Jet Propulsion Laboratory and the Seismological Laboratory, California Institute of Technology, and was sponsored by the Sun Oil Company, Ametek Corporation, and the National Aeronautics and Space Administration. Contribution 4249 of the Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena.
Funders:
Funding AgencyGrant Number
Sun Oil Co.UNSPECIFIED
Ametek CorporationUNSPECIFIED
NASAUNSPECIFIED
Subject Keywords:Seismology: Body waves; Seismology: Structure of the crust; Seismology: Structure of the lithosphere and upper mantle
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Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences4249
Record Number:CaltechAUTHORS:20121016-125457564
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20121016-125457564
Official Citation:Frankel, A. and R. W. Clayton (1986), Finite difference simulations of seismic scattering: Implications for the propagation of short-period seismic waves in the crust and models of crustal heterogeneity, J. Geophys. Res., 91(B6), 6465–6489, doi:10.1029/JB091iB06p06465.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34924
Collection:CaltechAUTHORS
Deposited By: Aucoeur Ngo
Deposited On:17 Oct 2012 23:11
Last Modified:27 Dec 2012 02:52

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