

Author: Gudkova T. Raevskii S.
Publisher: MAIK Nauka/Interperiodica
ISSN: 0038-0946
Source: Solar System Research, Vol.47, Iss.1, 2013-01, pp. : 11-19
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Abstract
The determination of the internal structure of the Moon using bulk waves is largely complicated due to inhomogeneities in its uppermost layer. We investigate the possibility of studying the Moon’s interior by a sensing method using the free oscillations of the Moon. The spectrum of the free oscillations is calculated for two current models of the internal structure of the Moon derived from the analysis of the
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