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Titlebook: Atmospheres and Ionospheres of the Outer Planets and Their Satellites; Sushil K. Atreya Book 1986 Springer-Verlag Berlin Heidelberg 1986 c

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11#
發(fā)表于 2025-3-23 10:58:44 | 只看該作者
12#
發(fā)表于 2025-3-23 14:52:20 | 只看該作者
Vertical Mixing,re . is the number density of the constituent, and . and . are respectively its molecular and eddy diffusion velocities. The latter can be expressed in terms of the density and thermal gradients (Colegrove et al. 1966), so that..
13#
發(fā)表于 2025-3-23 20:25:56 | 只看該作者
Candida: A Disease of Antibiotics,ce and nature of the other clouds are at this time simply postulated on theoretical grounds. Preliminary numerical simulation of the cloud structure on the major planets was done by Weidenschilling and Lewis (1973), whereas the results of the most recent calculations have been published by Atreya and Romani (1985).
14#
發(fā)表于 2025-3-24 00:47:52 | 只看該作者
Cloud Structure,ce and nature of the other clouds are at this time simply postulated on theoretical grounds. Preliminary numerical simulation of the cloud structure on the major planets was done by Weidenschilling and Lewis (1973), whereas the results of the most recent calculations have been published by Atreya and Romani (1985).
15#
發(fā)表于 2025-3-24 03:10:59 | 只看該作者
Book 1986scovery was significant not only in the context of Jupiter; it gave credence to and was instrumental in firmly establishing the heliocentric system of Nicolaus Copernicus. Almost four centuries after Galileo‘s discovery, exten- sive observations by the two Voyager spacecrafts have once again revolu-
16#
發(fā)表于 2025-3-24 08:02:24 | 只看該作者
17#
發(fā)表于 2025-3-24 10:59:09 | 只看該作者
Thermal Structure,s of basic planetary temperatures and radiative transfer are developed first, followed by principles of the most commonly used techniques for temperature determination on the major planets. Since considerably more information is presently available for Jupiter and Saturn, their results are treated s
18#
發(fā)表于 2025-3-24 17:55:48 | 只看該作者
Cloud Structure,ered cloud structure. On Jupiter, for example, the predicted clouds in the region of the Galileo/Probe descent are ammonia ice (NH.-ice), ammonium hydrosulfide crystals (NH.SH-s), and water-ice (H.0-ice) as illustrated in Fig. 1.5. On Uranus and Neptune, clouds of methane ice (CH.-ice) and aqueous a
19#
發(fā)表于 2025-3-24 22:53:39 | 只看該作者
20#
發(fā)表于 2025-3-25 03:08:01 | 只看該作者
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