Diurnal minima of the infrared brightness temperatures of Venus

Details Diurnal minima of the infrared brightness temperatures of Venus Diurnal minima of the infrared brightness temperatures of Venus

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..422k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, May-June 1979, p. 422-433. In Russian.

Astronomy and Astrophysics

Astronomy

Brightness Temperature, Diurnal Variations, Infrared Astronomy, Venus (Planet), Aerosols, Atmospheric Stratification, Extremum Values, Thermal Radiation, Venera Satellites, Venus Clouds

Scientific paper

Venera-9 and Venera-10 radiometer data were used to construct a generalized diagram of the diurnal distribution of the thermal emission intensity of Venus, reduced to a local vertical at each point of the planet's equatorial belt. A limb darkening analysis shows the existence of two states of the upper boundary of the emitting cloud layer, corresponding to day and night conditions. Observed minima of brightness temperature on the night side of the planet can be explained by attenuation of radiative fluxes by aerosol masses, formed in daytime photochemical reactions and situated in the colder layers of the atmosphere, above the principal cloud level.

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