Microstructure of the Venus cloud layer according to results of the Venera-11 spectrophotometric experiment

Details Microstructure of the Venus cloud layer according to results of the Venera-11 spectrophotometric experiment Microstructure of the Venus cloud layer according to results of the Venera-11 spectrophotometric experiment

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..120t&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, Jan.-Feb. 1984, p. 120-129. In Russian.

Computer Science

Sound

Aerosols, Atmospheric Sounding, Particle Size Distribution, Spectrophotometry, Venera 11 Satellite, Venus Clouds, Atmospheric Refraction, Cloud Cover, Satellite Sounding

Scientific paper

The cloud-particle size distribution at heights of 48-65 km was reconstructed on the basis of Venera-11 data using the Tikhonov regularization method. A combined interpretation of spectrophotometric and nephelometric data made it possible to determine the aerosol refractive index. A value of about 1.33, obtained for the lower part of the cloud layer, points to the possible presence of aspherical particles.

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