Modeling Ice Stability with Topography on a Local Scale, Mars

Details Modeling Ice Stability with Topography on a Local Scale, Mars Modeling Ice Stability with Topography on a Local Scale, Mars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1554r&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1554

Physics

1

Scientific paper

We model ice stability on a local scale, examining 1) the relative
importance of 4 energy-balance factors introduced by topography, 2) the
resulting spatial variation in ice stability, and 3) the resulting cycle
in which changes in surface shape depend on shape itself.

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