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Mariner-9 based simulation of radiative convective temperature changes in the Martian dust-laden atmosphere-soil system (1974)

Pallmann, A. J. ; Dannevik, W. P.

In: CASI

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Publication Date: 2019-06-27

Description: A numerical simulation of radiative, conductive, and convective heat transfer of the Martian dust-laden atmosphere-soil system is presented with particular emphasis given to heating/cooling in regions of sharp variation in temperature or absorption and its resultant impact on outgoing planetary spectral radiance, as measured by the Mariner 9 IRIS. Thermal coupling between the ground and atmospheric subsystems is modeled by the total heat flux balance at the interface. In the simulation procedure, local thermodynamic equilibrium (LTE) is assumed, and a combined strong-weak line transmission function permits short- and long-range exchanges of energy from the surface toward space. Direct absorption of insolation in the near-IR bands by both silicate dust and CO2 is incorporated.

Keywords: SPACE SCIENCES

Type: NASA-CR-138834

Format: application/pdf

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