Abstract

SUMMARY Since its beginning in acoustics, the Time-Reversal method (hereafter referred as TR) has been explored by different studies to locate and characterize seismic sources in elastic media. But few authors have proposed an analytical analysis of the method, especially in the case of an elastic medium and for a finite body such as the Earth. In this paper, we use a normal mode approach (for general 3-D case and degenerate modes in 1-D reference model) to investigate the convergence properties of the TR method. We first investigate a three-point problem, with two fixed points which are the source and the receiver and a third one corresponding to a changing observation point. We extend the problem of a single channel TR experiment to a multiple channel and multiple station TR experiment. We show as well how this problem relates to the retrieval of Green’s function with a multiple source cross-correlation and also the differences between TR method and cross-correlation techniques. Since most of the noise sources are located close to the surface of the Earth, we show that the time derivative of the cross-correlation of long-period seismograms with multiple sources at the surface is different from the Green’s function. Next, we show the importance of a correct surface-area weighting of the signal resent by the stations according to a Voronoi tessellation of the Earth surface. We use arguments based on the stationary phase approximation to argue that phase-information is more important than amplitude information for getting a good focusing in TR experiment. Finally, by using linear relationships between the time-reversed displacement (resp. strain wavefields) and the components of a vector force source (resp. a moment tensor source), we show how to retrieve force (or moment tensor components) of any long period tectonic or environmental sources by time reversal.

Highlights

  • Since its first applications in pure acoustics, the time-reversal approach (Fink 1997), has been extended to the 3-D elastic case

  • Eigenmode analysis has been used in the scalar case to investigate the limitation of TR in chaotic cavities (Draeger & Fink 1997, 1999) and for diffuse wavefields (Weaver & Lobkis 2002). We extend this approach using the normal mode theory for the 3-D elastic Earth

  • Normal mode theory is very convenient for addressing any scientific issue related to the global scale, since any displacement at the surface of the Earth can be expanded on the basis of normal mode eigenfunctions

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Summary

Introduction

Since its first applications in pure acoustics, the time-reversal approach (Fink 1997), has been extended to the 3-D elastic case. We extend this approach using the normal mode theory for the 3-D elastic Earth. Larmat et al (2006) showed that, when applied to the data of 2004 December 26 Sumatra-Andaman earthquake data, back-propagated waves focused at the right location and the right origin time of the epicentre, and made it possible to retrieve the source-time function, by using a simple normal mode summation code (Capdeville 2005) in a 1-D Earth model such as PREM (Dziewonski & Anderson 1981) at periods larger than 100s. The method has been implemented in 3-D-heterogeneous models and has been applied to locate glacial earthquakes (Larmat et al 2008), or tremors

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