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• W1990136242 abstract "Several photometric measurements of Venus made from the Pioneer Venus orbiter and probes indicate that solar near-ultraviolet radiation is being absorbed throughout much of the main cloud region, but little above the clouds or within the first one or two optical depths. Radiative transfer calculations were carried out to simulate both Pioneer Venus and ground-based data for a number of proposed cloud compositions. This comparison rules out models invoking nitrogen dioxide, meteoritic material, and volatile metals as the source of the ultraviolet absorption. Models involving either small ( approximately 1 micrometer) or large ( approximately 10 micrometers) sulfur particles have some serious difficulties, while ones invoking sulfur dioxide gas appear to be promising." @default.
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• W1990136242 date "1979-07-06" @default.
• W1990136242 modified "2023-09-27" @default.
• W1990136242 title "Nature of the Ultraviolet Absorber in the Venus Clouds: Inferences Based on Pioneer Venus Data" @default.
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• W1990136242 doi "https://doi.org/10.1126/science.205.4401.76" @default.
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