Photometry at 3500 A from Venera 9 and Venera 10

Details Photometry at 3500 A from Venera 9 and Venera 10 Photometry at 3500 A from Venera 9 and Venera 10

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..886k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 16, Nov.-Dec. 1978, p. 886-894. In Russian.

Physics

1

Aerosols, Diurnal Variations, Ultraviolet Photometry, Venera Satellites, Venus Atmosphere, Venus Clouds, Atmospheric Scattering, Atmospheric Stratification, Brightness, High Resolution, Rayleigh Scattering, Stratosphere

Scientific paper

In the present paper, some of the more interesting Venusian brightness profiles in the ultraviolet are presented and discussed. Measurements carried out near the morning and evening terminators of the planet point to the existence of a stratified nighttime cloud structure in the Venusian stratosphere. Measurements reveal an extended diffuse aerosol medium during daytime.

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