The Martian climate: Energy balance models with CO2/H2O atmospheres

Details The Martian climate: Energy balance models with CO2/H2O atmospheres The Martian climate: Energy balance models with CO2/H2O atmospheres

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984suny.rept.....h&link_type=abstract

Semiannual Status Report, 1 Mar. - 1 Sep. 1984 New York Univ., New York. Dept. of Applied Science.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Atmospheric Models, Climate, Long Wave Radiation, Mars (Planet), Mars Atmosphere, Mars Surface, Surface Temperature, Carbon Dioxide, Elastic Waves, Polar Regions, Seasons, Solar Radiation

Scientific paper

Progress in the development of a multi-reservoir, time dependent energy balance climate model for Mars driven by prescribed insolation at the top of the atmosphere is reported. The first approximately half-year of the program was devoted to assembling and testing components of the full model. Specific accomplishments were made on a longwave radiation code, coupling seasonal solar input to a ground temperature simulation, and conceptualizing an approach to modeling the seasonal pressure waves that develop in the Martian atmosphere as a result of sublimation and condensation of CO2 in polar regions.

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