The spectral and spatial structure of the thermal emission field in a turbid Mars atmosphere

Details The spectral and spatial structure of the thermal emission field in a turbid Mars atmosphere The spectral and spatial structure of the thermal emission field in a turbid Mars atmosphere

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975dossr.224..316k&link_type=abstract

Akademiia Nauk SSSR, Doklady, vol. 224, Sept. 11, 1975, p. 316-319. In Russian.

Astronomy and Astrophysics

Astronomy

Atmospheric Radiation, Dust Storms, Mars Atmosphere, Thermal Emission, Turbidity, Astronomical Models, Deep Scattering Layers, Planetary Radiation, Spectral Energy Distribution

Scientific paper

Turbidity in the Mars atmosphere is due to large-scale dust storms. In order to study this phenomenon and the spectral and spatial structure of the thermal emission field in the turbid Mars atmosphere a semi-infinite absorbing and scattering layer model is used. Numerical calculations are presented for obtaining the spectral intensities of ascending and descending thermal emission.

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