The Last 10 Myr on Mars: Comparing Atmospheric Simulations with Recent Geology

Details The Last 10 Myr on Mars: Comparing Atmospheric Simulations with Recent Geology The Last 10 Myr on Mars: Comparing Atmospheric Simulations with Recent Geology

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1818m&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1818

Mathematics

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Scientific paper

We develop a fully coupled, obliquity-driven linear model of the
evolution of Mars' CO_2 atmosphere. Correlations between program output
and recently emplaced layered geological features enable an
understanding the climate during recent "ice-ages".

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