Other
Scientific paper
Jul 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...80..202k&link_type=abstract
Icarus (ISSN 0019-1035), vol. 80, July 1989, p. 202-210.
Other
9
Atmospheric Composition, Chemical Composition, Vega Project, Venus Clouds, Aerosols, Chlorides, Phosphorus, Sulfur Dioxides, Sulfuric Acid, Venus, Vega Missions, Spacecraft Observations, Chemistry, Composition, Clouds, Physical Properties, Aerosols, Analysis, Mass Loading, Formation, Origin, Phosphorous, Phosphorous Anhydride, Evaporation, Photochemistry, Sulfur Dioxide, Sulfuric Acid, Ferric Chloride, Aluminum Chloride, Layers, X-Ray Methods, Fluorescence, Landing Sites, Landers, Comparisons, Structure
Scientific paper
Physical and chemical analyses of the clouds and atmosphere of Venus on the basis of Vega payload data have yielded a cloud-particle composition in which the presence of phosphoric acid straightforwardly accounts for the fact that the clouds extend down to the 33-km limit of Vega's spectrometric, nephelometric, and photometric instrumentation. Attention is given to the problem posed by the inconsistency of these results with the much lower or entirely absent phosphorus at other Venera and Pioneer Venus landing probe sites. P4O6 is the main phosphorus-bearing gas.
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