A Preliminary Inversion of Lunar Regolith Thickness Using Earth-Based 70-cm Arecibo Radar Observations

Details A Preliminary Inversion of Lunar Regolith Thickness Using Earth-Based 70-cm Arecibo Radar Observations A Preliminary Inversion of Lunar Regolith Thickness Using Earth-Based 70-cm Arecibo Radar Observations

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1506f&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1506

Physics

Scientific paper

In this study, a rigorous radar scattering model based on vector
radiative transfer theory and Earth-based 70-cm Arecibo radar data are
used to invert for regolith thickness over the lunar nearside
hemisphere.

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