Mechanisms of cloud layer formation in Venusian atmosphere

Details Mechanisms of cloud layer formation in Venusian atmosphere Mechanisms of cloud layer formation in Venusian atmosphere

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rpsct...2...77z&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 77 (SEE N88-16063 08-42) Transl. into ENGLISH from Doklady Akademii Na

Computer Science

Aerosols, Atmospheric Composition, Atmospheric Stratification, Photochemical Reactions, Venus Atmosphere, Venus Clouds, Atmospheric Chemistry, Night, Particle Density (Concentration), Time Response, Vega Project, Vertical Distribution

Scientific paper

Data on the aerosol component of the Venus atmosphere obtained on the nightside of the planet by the Vega 1 and 2 probes on 11 and 15 June 1985 are discussed. The data indicate that the cloud system of the Venus atmosphere on the nightside can be viewed as a thick layer of photochemical haze at altitudes of 46 to 60 km. At altitudes of 56 to 60 and 46.5 to 49.5 km, thick layers (tiers) were observed which form due to the coarsening of primary nuclei.

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