Physics – Optics
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..899k&link_type=abstract
Kosmicheskie Issledovaniia, vol. 18, Nov.-Dec. 1980, p. 899-906. In Russian.
Physics
Optics
1
Aerosols, Astronomical Spectroscopy, Cloud Cover, Light Scattering, Venera Satellites, Venus Atmosphere, Atmospheric Density, Atmospheric Optics, Onboard Equipment, Planetary Limb, Spectrometers, Turbulent Mixing, Venera 10 Satellite, Venera 9 Satellite
Scientific paper
Spectroscopic observations at the planetary limb were used to investigate the basic characteristics of aerosol in the Venus atmosphere above the clouds. At heights of 70-100 km, particle radius varied from 1 to 0.1-0.2 micron, particle number density varied from 100 to 0.1 per cu cm, particle mass density varied from 10 to the -9th to 10 to the -15th g/cu cm, and relative sulfuric acid content varied from 10 to the -6th to 5 x 10 to the -9th. The turbulent mixing coefficient was 10,000 sq cm/s at 70-75 km and increased to 1-million to 10-million sq cm/s. Spectroscopic limits for the content of seven constituents at various heights are obtained.
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