Rugged Flow Morphology of Lunar Domes Revealed by Earth-based Radar

Details Rugged Flow Morphology of Lunar Domes Revealed by Earth-based Radar Rugged Flow Morphology of Lunar Domes Revealed by Earth-based Radar

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1299c&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

Scientific paper

New radar data show that domes in the Marius Hills region have
backscatter strength comparable to near-rim ejecta from young craters,
and circular polarization ratio values similar to blocky terrestrial
volcanic deposits like SP flow in Arizona.

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