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- W2007489151 abstract "Spectra of Uranus' S3(0) and S3(1) H2 quadrupole lines, obtained during the 1978-1980 apparitions, are analyzed, and are found to require the presence of a deep cloud. Modifications of the Baines and Bergstralh (1986) standard model, including an additional haze layer above the 16-km-am H2 level which contains strongly absorbing particles, are needed to fit the observations. For a Rayleigh phase function, such a haze (uniformly mixed with the gas above this level) would have an absorption optical depth of 0.16 and a single scattering particle albedo of 0.30. This modification would imply a fraction of normal H2 equal to 0.25 + or - 0.10, in agreement with the Baines and Bergstralh standard model." @default.
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- W2007489151 date "1987-04-01" @default.
- W2007489151 modified "2023-09-27" @default.
- W2007489151 title "Uranus' (3-0) H2 quadrupole line profiles" @default.
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- W2007489151 doi "https://doi.org/10.1016/0019-1035(87)90071-6" @default.
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