Reinterpretation of Mariner 9 IRIS data on the basis of a simulation of radiative-conductive convective transfer in the dust laden Martian atmosphere

Details Reinterpretation of Mariner 9 IRIS data on the basis of a simulation of radiative-conductive convective transfer in the dust laden Martian atmosphere Reinterpretation of Mariner 9 IRIS data on the basis of a simulation of radiative-conductive convective transfer in the dust laden Martian atmosphere

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974slu..rept.....p&link_type=abstract

Final Report, Oct. 1973 - Dec. 1974 Saint Louis Univ., MO.

Physics

Conductive Heat Transfer, Convective Heat Transfer, Iris Satellites, Mariner 9 Space Probe, Mars Atmosphere, Radiative Heat Transfer, Algorithms, Atmospheric Models, Carbon Dioxide, Dust, High Resolution, Temperature Measurement

Scientific paper

Time dependent vertical distributions of atmospheric temperature and static stability were determined by a radiative-convective-conductive heat transfer model attuned to Mariner 9 IRIS radiance data. Of particular interest were conditions of both the dust-laden and dust-free atmosphere in the middle latitudes on Mars during the late S.H. summer season. The numerical model simulates at high spatial and temporal resolution (52 atmospheric and 30 subsurface levels; with a time-step of 7.5 min.) the heat transports in the ground-atmosphere system. The algorithm is based on the solution of the appropriate heating rate equation which includes radiative, molecular-conductive and convective heat transfer terms. Ground and atmosphere are coupled by an internal thermal boundary condition.

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