Spectroscopy of Jupiter - 3200 to 11,200 A.
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Pilcher, C. B.↗
Engineering topics
Prinn, R. G.
Publications and source records attributed to Prinn, R. G..
Uranus atmosphere - Structure and composition.
The best available data on the geometric albedo of Uranus are shown to be compatible with a model in which particulate matter is present in the atmosphere. Cloud structures compatible with simple models for the accretion of Uranus and with thermal-balance studies of its atmosphere are discussed. A methane haze layer is suggested by the observations, and a deep, dense ammonia cloud layer far below the methane clouds is considered likely.
Prinn, R. G.↗
Photochemistry of HCl and other minor constituents in the atmosphere of Venus
Venusian photochemistry, discussing hydrogen source from HCl, loss of water in relation to HCl, carbon dioxide stability and COS and hydrogen sulfide in visible clouds
Prinn, R. G.↗