Mathematics
Scientific paper
Mar 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994lpi....25..517h&link_type=abstract
In Lunar and Planetary Inst., The Twenty-Fifth Lunar and Planetary Science Conference. Part 2: H-O p 517-518 (SEE N94-36136 11-9
Mathematics
Air Land Interactions, Albedo, Atmospheric Effects, Atmospheric Models, Dust, Mars Atmosphere, Mars Surface, Thermal Emission, Thermal Mapping, Carbon Dioxide, Heat Transfer, Insolation, Land Surface Temperature, Mathematical Models, Opacity, Planetary Mapping
Scientific paper
The most widely used thermal inertia data for Mars assumes the atmospheric contribution is constant and equal to 2 percent of the maximum solar insolation. Haberle and Jakosky investigated the effect of including a dusty CO2 atmosphere and sensible heat exchange with the surface on thermal inertia. We recently utilized Haberle and Jakosky's coupled surface-atmosphere model to investigate the effects of such an atmosphere on the thermally derived albedo. The thermally derived albedo is the albedo which, together with the thermal inertia, provides model surface temperatures which best match the observed temperatures. New maps are presented of thermal inertia and thermally derived albedo which incorporate dust opacities derived from IRTM data.
Haberle Robert M.
Hayashi Joan N.
Jakosky Bruce M.
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