Analysis of the possibilities to determine lunar soil characteristics with the help of bistatic radar


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Abstract

An opportunity of determining the lunar soil characteristics via bistatic radar involving high-power ground-based transmitters operating in meter and decameter wave ranges and receivers located aboard Moon satellite is analyzed. Direct and inverse problems concerning stratified soil sounding to a large depth, as well as algorithms for determining the regolith layer thickness, permittivity, radio wave absorption, and regolith and bedrock densities, are examined.

About the authors

O. V. Yushkova

Kotel’nikov Institute of Radio Engineering and Electronics (Fryazino Branch)

Author for correspondence.
Email: o.v.y@mail.ru
Russian Federation, Fryazino, Moscow oblast, 141190

O. I. Yakovlev

Kotel’nikov Institute of Radio Engineering and Electronics (Fryazino Branch)

Email: o.v.y@mail.ru
Russian Federation, Fryazino, Moscow oblast, 141190

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