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- W7883695 abstract "Data about the cyclic conversions of sulfur-containing gases in the atmosphere of Venus are generalized. Possible ways of fixing sulfur in the planet's crust are discussed, and the distinguishing features of the sulfur cycle in the outer layers of the Earth and Venus are indicated. The fast atmospheric sulfur cycle determines the existence of a continuous cloud cover of liquid H/sub 2/SO/sub 4/ aerosols right up to a height of approx. 85 km. At the levels from 47 to 49 km above the planet's surface, the condensates of H/sub 2/SO/sub 4/ are subjected to thermal dissociation, and the SO/sub 3/ which is formed here is reduced to CO/sub 2/ by carbon monoxide. The time a SO/sub 2/ molecule stays in the fast sulfur cycle is estimated to be a time interval from several days in the stratosphere to several years (the lifetime of the largest cloud particles) in the lower cloud layers." @default.
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- W7883695 date "1987-10-01" @default.
- W7883695 modified "2023-09-26" @default.
- W7883695 title "Scheme of the sulfur cycle in the outer layers of the planet Venus" @default.
- W7883695 hasPublicationYear "1987" @default.
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