標(biāo)題: Titlebook: Atmospheres and Ionospheres of the Outer Planets and Their Satellites; Sushil K. Atreya Book 1986 Springer-Verlag Berlin Heidelberg 1986 c [打印本頁] 作者: minuscule 時間: 2025-3-21 18:38
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作者: 合適 時間: 2025-3-21 22:00
Book 1986attained suf- ficient maturity to warrant a monograph of its own. Second, I have felt that as a result of recent observations, new and challenging problems have arisen whose resolution requires unconventional analysis and theoretical interpreta- tion of existing data, as well as the collection of ne作者: 抒情短詩 時間: 2025-3-22 02:17 作者: Deject 時間: 2025-3-22 05:39 作者: 小溪 時間: 2025-3-22 09:19 作者: 不再流行 時間: 2025-3-22 12:56
Satellites,ely tenuous atmospheres might also exist on some of the Galilean moons (Europa, Ganymede, and Callisto), and above the rings of Saturn. Io’s atmosphere seems to result from its perpetual volcanic activity caused by its unique tidal interaction in the Jovian system. The ability of Titan to retain an 作者: pineal-gland 時間: 2025-3-22 17:41
Felipe San-Blas,Gioconda San-Blasan thermal velocity (Appendix A1.1) of hydrogen atoms at Jupiter’s exospheric temperature (～1000K) is only 4 kms.. The time constant (also known as the e-folding time) for hydrogen atoms, i.e., the time required for escape of ～70% of the total atmospheric hydrogen, turns out to be 10. years! Nonther作者: gangrene 時間: 2025-3-23 00:18
Arti Gupta,Nagendra Pratap Singhtospheric hazes. On Jupiter and Saturn, NH. forms a visible cloud. Its saturated vapor abundance above the clouds, however, is large enough for it to be photolyzed as well. For all practical purposes, the NH. photochemistry is both spectroscopically and physically separated from the CH. photochemist作者: Mercurial 時間: 2025-3-23 04:35
https://doi.org/10.1007/978-94-011-0693-1ely tenuous atmospheres might also exist on some of the Galilean moons (Europa, Ganymede, and Callisto), and above the rings of Saturn. Io’s atmosphere seems to result from its perpetual volcanic activity caused by its unique tidal interaction in the Jovian system. The ability of Titan to retain an 作者: 新義 時間: 2025-3-23 06:12
0079-1938 10. The discovery 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 aga作者: 一加就噴出 時間: 2025-3-23 10:58 作者: blithe 時間: 2025-3-23 14:52
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..作者: monogamy 時間: 2025-3-23 20:25
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).作者: Classify 時間: 2025-3-24 00:47
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).作者: PACT 時間: 2025-3-24 03:10
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-作者: Intruder 時間: 2025-3-24 08:02 作者: 鳴叫 時間: 2025-3-24 10:59
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作者: 使長胖 時間: 2025-3-24 17:55
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作者: 閑逛 時間: 2025-3-24 22:53 作者: 治愈 時間: 2025-3-25 03:08 作者: Adenocarcinoma 時間: 2025-3-25 07:10
Ionosphere,ger spacecrafts. The principal difference between the Pioneer and the Voyager measurements is that the former were carried out using a single frequency oscillator (S-band at 2.293 GHz or 13 cm-.), while the latter employed dual frequency mode (S-band, and X-band at 8.6 GHz or 3.6 cm-.).作者: 服從 時間: 2025-3-25 10:31 作者: arabesque 時間: 2025-3-25 11:38 作者: Banister 時間: 2025-3-25 18:02 作者: curriculum 時間: 2025-3-25 23:05
https://doi.org/10.1007/978-3-030-69507-1ger spacecrafts. The principal difference between the Pioneer and the Voyager measurements is that the former were carried out using a single frequency oscillator (S-band at 2.293 GHz or 13 cm-.), while the latter employed dual frequency mode (S-band, and X-band at 8.6 GHz or 3.6 cm-.).作者: GEST 時間: 2025-3-26 03:23
https://doi.org/10.1007/978-3-642-71394-1chemistry; planet; solar system作者: 憤怒歷史 時間: 2025-3-26 08:18 作者: floodgate 時間: 2025-3-26 11:06
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 separately from Uranus and Neptune.作者: 小鹿 時間: 2025-3-26 13:51 作者: 不可侵犯 時間: 2025-3-26 17:43
Felipe San-Blas,Gioconda San-Blasense cloud of dust and gas surrounding the juvenile Sun. The Sun and its planetary system represent perhaps only one of the thousands of fragments which may have resulted following the collapse of a large interstellar cloud. According to the above hypothesis of solar system formation, the constituen作者: 青石板 時間: 2025-3-27 00:17 作者: 吞沒 時間: 2025-3-27 03:29
Candida: A Disease of Antibiotics,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作者: 膽汁 時間: 2025-3-27 07:37
https://doi.org/10.1057/9781137377029 respectively production and chemical loss rates per unit volume, and . is the vertical flux of the . constituent. . obeys the diffusion equation,.where . is the number density of the constituent, and . and . are respectively its molecular and eddy diffusion velocities. The latter can be expressed i作者: Etching 時間: 2025-3-27 13:26
Arti Gupta,Nagendra Pratap Singhhe recycling of CH. and NH. following their photodecomposition. Numerous minor constituents are produced in a planetary atmosphere, predominantly by photochemical processes, subsequent to the absorption of solar ultraviolet photons by various atmospheric molecules. The knowledge of the distribution 作者: Slit-Lamp 時間: 2025-3-27 17:28 作者: LAP 時間: 2025-3-27 19:39
https://doi.org/10.1007/978-94-011-0693-1 velocity. As a consequence, any volatiles outgassed during and after the accretionary phase of the moons would be rapidly lost. Since the conventional dynamo mechanism does not operate on the moons, they do not possess intrinsic magnetic fields. Therefore, they are likely to be stripped of any rema作者: 按時間順序 時間: 2025-3-27 22:20
Physics and Chemistry in Spacehttp://image.papertrans.cn/b/image/164600.jpg作者: 調(diào)情 時間: 2025-3-28 04:16 作者: 愚蠢人 時間: 2025-3-28 10:12
