A numerical simulation of climate changes during the obliquity cycle on Mars

Details A numerical simulation of climate changes during the obliquity cycle on Mars A numerical simulation of climate changes during the obliquity cycle on Mars

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9514761f&link_type=abstract

(American Geophysical Union and Geological Society of America, International Conference on Mars, 4th, Tucson, AZ, Jan. 10-13, 19

Mathematics

Logic

21

Carbon Dioxide Concentration, Climate Change, Digital Simulation, Mars Atmosphere, Planetary Meteorology, Polar Caps, Diurnal Variations, Greenhouse Effect, Heat Transfer, Mars Surface, Solar Radiation

Scientific paper

A one-dimensional seasonal energy balance climate model of the Martian surface is developed. The model shows the importance of using short-period diurnal and seasonal variations of solar irradiance instead of yearly-averaged quantities. The roles of meridional heat transport and greenhouse warming are shown to be important. The possible existence of hysteresis cycles in the formation and sublimation of permanent deposits during the course of the obliquity cycle is demonstrated.

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