Physics
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1025c&link_type=abstract
33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1025
Physics
Scientific paper
DEMs, made using the Magellan Stereo Toolkit, and F-Map images of 3
craters are analysed to show that their dark features are most probably
caused by fine sediment lying in depressions rather than lava.
Cochrane Christopher G.
Ghail Richard C.
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