Other
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...57..143t&link_type=abstract
Icarus (ISSN 0019-1035), vol. 57, Feb. 1984, p. 143-160.
Other
19
Atmospheric Composition, Particle Size Distribution, Planetary Composition, Venus Clouds, Instrument Errors, Pioneer Venus Spacecraft, Planetology, Solids, Spectrometers, Sulfuric Acid, Venera Satellites, Venus Atmosphere, Venus, Clouds, Particles, Pioneer Venus, Abundance, Size, Spectrometer, Techniques, Analysis, Sulfuric Acid, Distribution, Venera Missions, Optical Properties, Refractive Index, Sulfur, Atmosphere
Scientific paper
The discovey of large, solid particles in the clouds of Venus is one of the most significant findings of Pioneer Venus because it means that a substantial mass of the clouds is composed of a material other than sulfuric acid. The evidence which suggests that solid particles form a distinctive size mode is reexamined. It is shown that all of the Pioneer Venus and Venera optical data from the lower clouds can be explained with sulfuric acid droplets without introducing any solid particles. As a by-product of this analysis, it is also found that the upper clouds of Venus must contain a material with a higher refractive index than sulfuric acid. A small quantity of sulfur could account for this observation.
Blamont Jacques
Colburn D.
Cot Charles
Ragent Boris
Toon Brian O.
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