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Temporal changes in the lunar soil from correlation of diffuse vibrations

Christoph Sens-Schönfelder and Eric Larose
Phys. Rev. E 78, 045601(R) – Published 22 October 2008
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Abstract

It was recently demonstrated that one can reconstruct the impulse response between passive sensors by cross-correlating diffuse waves or ambient noise. Using seismic waves recorded on the moon, we show here that not only direct waves can be retrieved, but also late arrivals that have been scattered before reaching the seismometers. As these late arrivals propagate for a longer time, they are more sensitive to weak perturbations of the medium such as velocity changes. This high sensitivity of scattered waves is used to monitor periodic velocity changes in the lunar soil by measuring small delays of the passively retrieved coda waves. The velocity changes result from temperature variations due to periodic heating of the lunar surface by the sun.

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  • Received 17 March 2008

DOI:https://doi.org/10.1103/PhysRevE.78.045601

©2008 American Physical Society

Authors & Affiliations

Christoph Sens-Schönfelder*

  • Institute for Geophysics and Geology, Universität Leipzig, Talstraße 35, 04103 Leipzig, Germany

Eric Larose

  • Laboratoire de Géophysique Interne et Tectonophysique, Université Joseph Fourier and CNRS, Grenoble France BP 53, 38041 Grenoble cedex 9, France

  • *Also at LGIT, Université Joseph Fourier. sens-schoenfelder@uni-leipzig.de

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Issue

Vol. 78, Iss. 4 — October 2008

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