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• W2053635325 abstract "Abstract Spectrophotometry of Venus from 2170 to about 1950 A has been obtained by OAO-2 at 10 A resolution. The new data confirm and extend previous indications that the geometric albedo decreases continuously below 2500 A. Secular changes in either the amount or distribution, or both, of absorbing constituents in the upper atmosphere are strongly suggested. A narrow absorption feature is found near 2145 A, confirming an earlier report by Anderson et al. [ J. Atmos. Sci. 26 (1969), 874–888]. Absorption by trace amounts of nitrogen-bearing molecules, including N 2 O, HNO 3 in aqeous solution, and possibly also NO, together with Rayleigh scattering from CO 2 , can account for the variation in albedo below 3200 A, but other explanations are not excluded. For example, H 2 S may contribute to or be responsible for the decrease in albedo below 2500 A." @default.
• W2053635325 created "2016-06-24" @default.
• W2053635325 creator A5035617115 @default.
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• W2053635325 date "1976-02-01" @default.
• W2053635325 modified "2023-09-24" @default.
• W2053635325 title "Photometry of Venus below 2200 Å from the orbiting astronomical observatory-2" @default.
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• W2053635325 doi "https://doi.org/10.1016/0019-1035(76)90008-7" @default.
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