Diurnal Forcing of Planetary Atmospheres

Details Diurnal Forcing of Planetary Atmospheres Diurnal Forcing of Planetary Atmospheres

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995stin...9621452h&link_type=abstract

Technical Report, Space Physics Research Inst. ,Sunnyvale,CA United States

Mathematics

Logic

Mars Environment, Atmospheric General Circulation Models, Hydrological Cycle, Climate Models, Atmospheric Circulation, Computerized Simulation, Planetary Atmospheres, Transport Properties, Soils, Stratosphere, Aerosols, Boundary Conditions, Water Vapor, Polar Caps, Volcanoes, Earth Atmosphere

Scientific paper

The Mars Climate Model developed by the Ames Research Center is a unique tool for the study of longterm atmospheric transport on both the Earth and Mars. This computer model combines the full dynamics of an atmospheric general circulation model, a sophisticated tracer transport scheme, a full hydrological cycle, and a subsurface soil model. In its terrestrial application, the model combines a stratospheric general circulation model with the same tracer transport scheme, a specialized lower boundary condition forcing procedure, data assimilation capabilities, and aerosol microphysical modeling.

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