Gaseous sulfur in the Venusian atmosphere

Details Gaseous sulfur in the Venusian atmosphere Gaseous sulfur in the Venusian atmosphere

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..600s&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, July-Aug. 1980, p. 600-608. In Russian.

Computer Science

6

Atmospheric Composition, Solar Radiation, Sulfur, Vapor Phases, Venera Satellites, Venus Atmosphere, Absorption Spectra, Allotropy, Atmospheric Models, Lower Atmosphere, Partial Pressure, Spectrophotometers, Vertical Distribution

Scientific paper

It is shown that the increased extinction of solar radiation scattered in the Venusian atmosphere, recorded by scanning spectrophotometers on board Venera 11 and 12, may be explained by the presence of gaseous sulfur in the lower atmosphere of the planet. A model of the vertical distribution of gaseous sulfur with respect to allotropic states is proposed.

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