Effective mie-scattering and CO2 absorption in the dust-laden Martian atmosphere and its impact on radiative-convective temperature changes in the lower scale heights

Details Effective mie-scattering and CO2 absorption in the dust-laden Martian atmosphere and its impact on radiative-convective temperature changes in the lower scale heights Effective mie-scattering and CO2 absorption in the dust-laden Martian atmosphere and its impact on radiative-convective temperature changes in the lower scale heights

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976slu..rept.....p&link_type=abstract

Final Report, Dec. 1974 - Mar. 1976 Saint Louis Univ., MO. Dept. of Earth and Atmospheric Sciences.

Mathematics

Atmospheric Attenuation, Atmospheric Temperature, Carbon Dioxide, Mars Atmosphere, Mie Scattering, Molecular Absorption, Computerized Simulation, Dust, Heat Transfer, Infrared Radiometers, Mathematical Models, Particulates, Planetary Surfaces, Radio Occultation, Spectrum Analysis

Scientific paper

A time dependent computer model of radiative-convective-conductive heat transfer in the Martian ground-atmosphere system was refined by incorporating an intermediate line strength CO2 band absorption which together with the strong-and weak-line approximation closely simulated the radiative transmission through a vertically inhomogeneous stratification. About 33,000 CO2 lines were processed to cover the spectral range of solar and planetary radiation. Absorption by silicate dust particulates, was taken into consideration to study its impact on the ground-atmosphere temperature field as a function of time. This model was subsequently attuned to IRIS, IR-radiometric and S-band occultation data. Satisfactory simulations of the measured IRIS spectra were accomplished for the dust-free condition. In the case of variable dust loads, the simulations were sufficiently fair so that some inferences into the effect of dust on temperature were justified.

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