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- W2003223485 abstract "Abstract The present status of research on the composition of planetary atmospheres is reviewed. It is shown that CO 2 is the major constituent in the atmospheres of Venus and Mars, and that H 2 is almost certainly the dominant constituent for the outer planets Jupiter, Saturn, Uranus, and Neptune. Ground based i.r. spectroscopy is the largest single source of information on atmospheric composition and much of the paper is concerned with difficulties involved in the interpretation of i.r. spectra. The mechanisms for line formation are examined carefully and it is concluded that multiple scattering by cloud materials must play a dominant role for Jupiter, Saturn, and Venus. There is no evidence for visible cloud layers on either Uranus or Neptune. Both planets, however, exhibit deep molecular atmospheres and Rayleigh scattering will affect the strength of absorption features. Considerable attention is given to the techniques available for the line formation problem in a scattering medium, and the usefulness of similarity relations is emphasized. The dependence of equivalent width on abundance and pressure is obscure for a scattering atmosphere. The principal characteristics of the scattering curve of growth are reviewed from an intuitive rather than mathematical viewpoint." @default.
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- W2003223485 date "1971-06-01" @default.
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- W2003223485 title "The composition of planetary atmospheres" @default.
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- W2003223485 doi "https://doi.org/10.1016/0022-4073(71)90058-6" @default.
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