Solar radiation scattered in the Venus atmosphere - The Venera 11, 12 data

Details Solar radiation scattered in the Venus atmosphere - The Venera 11, 12 data Solar radiation scattered in the Venus atmosphere - The Venera 11, 12 data

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...53..509m&link_type=abstract

Icarus (ISSN 0019-1035), vol. 53, March 1983, p. 509-537.

Astronomy and Astrophysics

Astronomy

16

Astronomical Spectroscopy, Solar Radiation, Solar Spectra, Spaceborne Astronomy, Venus Atmosphere, Venus Clouds, Atmospheric Composition, Data Acquisition, Satellite-Borne Instruments, Solar Flux, Venera 11 Satellite, Venera 12 Satellite, Venus, Atmosphere, Solar Radiation, Scattering, Venra 11, Venera 12, Spectra, Probes, Spectrometry, Photometry, Flux, Absorption, Size, Landing Sites, Clouds, Layers, Structure, Optical Properties, Depth, Wavelengths, Particles, Sulfer, Mixing Ratio

Scientific paper

Venera 11 and 12 probe measurements of scattered solar radiation in the Venus atmosphere are presented. The integral downward solar radiation flux toward the surface near the Venera 11 landing site was 78 W/sq m, and the value of the downward solar flux on the surface at the subsolar point, averaged over the data from several probes, is 90 + or - 12 W/sq m. The lower boundary layer of Venus is found to be at a height of about 48 km at the landing sites of both of the present probes. The structure of the investigated region of the cloud layer, at 48-63 km altitude, is almost identical and consists of three parts with boundaries between them at about 51 and 57 km.

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