Mucosa 发表于 2025-3-23 12:44:56
Nature of the Venus Clouds as Derived from Their Polarization particle properties deduced from the polarization eliminate all but one of the cloud compositions which have been proposed for Venus. A concentrated solution of sulfuric acid (H.SO.-H.O) provides good agreement with the polarization data.cinder 发表于 2025-3-23 15:16:36
Water Vapor in Venus Determined by Airborne Observations of the 8200 Å Bandlution groundbased studies..These results establish that the average value over the entire disk is quite low but allows that locally larger values may exist as reported by Barker. A more complete description of this work appeared in . . (1974), 213.织物 发表于 2025-3-23 20:50:00
Book 1974 of his birth, came during the XIV General Assembly of IAU in Brighton. The Executive Committee has approved it in the program of the Extraordinary (Copernicus) General Assembly ofIAU in Poland in 1973. The IAU Symposium No 65 (Copernicus Symposium IV) on the ‘Exploration of the Planetary System‘ wa大都市 发表于 2025-3-24 01:20:29
Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebulans of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volatile compounds, and the ‘optical’ properties of the grain-gas medium. A summary of available and still needed basic (input) data and some currently available results are presented.Inkling 发表于 2025-3-24 03:25:31
http://reply.papertrans.cn/32/3194/319395/319395_15.pngamplitude 发表于 2025-3-24 07:40:20
http://reply.papertrans.cn/32/3194/319395/319395_16.pngfrozen-shoulder 发表于 2025-3-24 13:53:06
http://reply.papertrans.cn/32/3194/319395/319395_17.pngintuition 发表于 2025-3-24 18:18:28
http://reply.papertrans.cn/32/3194/319395/319395_18.png类人猿 发表于 2025-3-24 21:26:13
http://reply.papertrans.cn/32/3194/319395/319395_19.pngadj忧郁的 发表于 2025-3-24 23:31:17
Robert W. Baloh,Robert E. BartholomewWe have searched for molecular lines in planetary atmospheres using the PEPSIOS spectrometer with an instrumental width about equal to that of the expected absorption line, and in the case of Jupiter, with the additional feature of Doppler compensation over the planetary disc.