Preliminary Regional Analysis of the Kaguya Lunar Radar Sounder (LRS) Data Through Eastern Mare Imbrium

Details Preliminary Regional Analysis of the Kaguya Lunar Radar Sounder (LRS) Data Through Eastern Mare Imbrium Preliminary Regional Analysis of the Kaguya Lunar Radar Sounder (LRS) Data Through Eastern Mare Imbrium

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2406a&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Computer Science

Sound

Scientific paper

We processed preliminary Kaguya Lunar Radar Sounder data to form a
coarse 3D voxel grid model. This model shows topography, a regional
boundary at ~3.8 km depth (but dipping to ~4.4 km in SE Mare Imbrium),
and the probable detection limits of the instrument at ~6.3 km depth.

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