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- W2146249360 abstract "As a necessary background for discussion of future prospects this review attempts to summarize current knowledge on observational data relating to the properties of planets at radio wavelengths. According to Whitcomb et al (Icarus, 1979, 38, 75), a consensus has emerged among the observers that “measurements of planetary brightness temperatures at wavelengths between 200 μm and 2 mm are of practical value in submillimeter astronomy since the planets are used as calibration sources in studies of other objects. In addition, such measurements can provide tests for theories of planetary atmospheres”. Although the former topic deserves great consideration, only the latter is developed here with special emphasis on the most recent observations of planets in the millimeter and submillimeter range. I briefly outline some major observational perspectives which embody very attractive goals of future planetary research." @default.
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- W2146249360 date "1996-01-01" @default.
- W2146249360 modified "2023-09-27" @default.
- W2146249360 title "Study of planetary atmospheres" @default.
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- W2146249360 doi "https://doi.org/10.1007/978-3-540-69999-6_45" @default.
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