Mars 2, 21-45, 2006 | doi:10.1555/mars.2006.0003
Received September 29, 2005 | Accepted May 29, 2006 | Published August 18, 2006
A comparison of terrestrial ice surfaces and martian layer bed surfaces provides insight into the history of polar processes. We identify a number of important observations of physical characteristics that future polar surface missions should make to help characterize deposits and distinguish among hypotheses.
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