Numerical modeling of radiative heat transfer in the atmospheres of Venus and Mars

Details Numerical modeling of radiative heat transfer in the atmospheres of Venus and Mars Numerical modeling of radiative heat transfer in the atmospheres of Venus and Mars

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979dossr.244q1334k&link_type=abstract

Akademiia Nauk SSSR, Doklady, vol. 244, Feb. 21, 1979, p. 1334-1336. In Russian.

Astronomy and Astrophysics

Astronomy

Computerized Simulation, Mars Atmosphere, Radiative Heat Transfer, Thermal Simulation, Venus Atmosphere, Astronomical Spectroscopy, Pressure Distribution, Temperature Distribution

Scientific paper

Spectral intensities of thermal radiation in the Venusian and Martian atmospheres are solved by the computer modeling of radiative transfer in absorbing gaseous media with nonuniform temperature and pressure distributions. Spectral intensities are calculated for a spherical atmosphere, taking into account the radiation characteristics of the principal component (CO2), of the minor constituents (water vapor, CO, NH3, HCl, and HF), and of the aerosol component.

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