Ultraviolet photometry of Venus - Scattering layer over absorbing clouds

Details Ultraviolet photometry of Venus - Scattering layer over absorbing clouds Ultraviolet photometry of Venus - Scattering layer over absorbing clouds

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976kosis..14..776k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 14, Sept.-Oct. 1976, p. 776-788. In Russian.

Physics

Optics

2

Light Scattering, Planetary Radiation, Ultraviolet Photometry, Venera Satellites, Venus Clouds, Astronomical Photometry, Atmospheric Optics, Atmospheric Stratification, Brightness Temperature, Cloud Cover, Satellite-Borne Instruments

Scientific paper

The basic aims of the UV photometry (in the range 3300-8000 A) of the Venus atmosphere from the Venera 9 and 10 probes was to study light scattering in the cloudy layers of the atmosphere, and in layers above the clouds, to measure contrasts, and to investigate the structure of the upper part of the cloud layer and the nature of dark and light formations. Photometry was directed at the upper tier of the cloud cover of Venus whose boundary is at a height of 64-67 km.

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