Volatile-rich Crater Interior Deposits on Mars: An Energy Balance Model of Modification

Details Volatile-rich Crater Interior Deposits on Mars: An Energy Balance Model of Modification Volatile-rich Crater Interior Deposits on Mars: An Energy Balance Model of Modification

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1249r&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1249

Physics

3

Scientific paper

We test the hypothesis that asymmetries in morphology and location of
volatile-rich deposits within craters result from asymmetries in local
energy balance due mainly to spatial variability of solar insolation and
radiative effects of crater walls.

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