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| Lunar noise correlation, imaging and monitoring |
| Christoph Sens-Schonfelder1, Eric Larose2 |
1 Institute for Geophysics and Geology, Universit?t Leipzig, 04103 Leipzig, Germany
2 Laboratoire de Géophysique Interne et Tectonophysique, CNRS and Université Joseph Fourier, 38041 Grenoble, France |
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Abstract Passive seismic techniques have revolutionarised seismology, leading for example to increased resolution in surface wave tomography, to the possibility to monitor changes in the propagation medium, and to many new processing strategies in seismic exploration. Here we review applications of the new techniques to a very particular dataset, namely data from the Apollo 17 lunar network. The special conditions of the lunar noise environment are investigated, illustrating the interplay between the properties of the noise and the ability to reconstruct Green’s functions. With a dispersion analysis of reconstructed Rayleigh waves new information about the shallow shear velocity structure of the Moon are obtained. Passive image interferometry is used to study the effect of temperature changes in the subsurface on the seismic velocities providing direct observation of a dynamic process in the lunar environment. These applications highlight the potential of passive techniques for terrestrial and planetary seismology.
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Received: 04 June 2010
Published: 10 October 2010
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Corresponding Authors:
Christoph Sens-Schonfelder
E-mail: sens-schoenfelder@uni-leipzig.de
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