The effects of nonideal surfaces on the derived thermal properties of Mars

Details The effects of nonideal surfaces on the derived thermal properties of Mars The effects of nonideal surfaces on the derived thermal properties of Mars

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.8252j&link_type=abstract

Journal of Geophysical Research, vol. 84, Dec. 30, 1979, p. 8252-8262.

Physics

19

Brightness Temperature, Mars Surface, Surface Properties, Surface Temperature, Thermal Mapping, Viking Mars Program, Atmospheric Pressure, Diurnal Variations, Infrared Detectors, Landing Sites, Mathematical Models

Scientific paper

The paper examines the effects of the observed brightness temperatures and the derived thermal inertias of some of the nonideal properties of the Martian surface. Attention is given to thermal models used for calculating the temperatures of the ideal and nonideal surfaces. Surfaces temperatures and derived thermal inertias for the various nonideal surfaces are presented. In addition, discussion covers the application of these models to the surface of Mars, the VL-1 landing site, the caldera atop Arsia Mons volcano, and the global relationships between thermal inertia and surface elevation.

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