Evolution of Volatile-rich Crater Interior Deposits on Mars

Details Evolution of Volatile-rich Crater Interior Deposits on Mars Evolution of Volatile-rich Crater Interior Deposits on Mars

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3256r&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3256

Computer Science

3

Scientific paper

We employ an energy balance approach to model the evolution of
volatile-rich crater interior deposits. Asymmetries due to crater
geometry and insolation patterns are compared with fill morphology at
the north and south poles.

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