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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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發(fā)表于 2025-3-21 18:38:01 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Atmospheres and Ionospheres of the Outer Planets and Their Satellites
影響因子2023Sushil K. Atreya
視頻videohttp://file.papertrans.cn/165/164600/164600.mp4
學科分類Physics and Chemistry in Space
圖書封面Titlebook: Atmospheres and Ionospheres of the Outer Planets and Their Satellites;  Sushil K. Atreya Book 1986 Springer-Verlag Berlin Heidelberg 1986 c
影響因子One of the most fundamental discoveries of the solar system was the detection of four moons in orbit around Jupiter by Galileo Galilei in 1610. 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 again revolu- tionized our thinking about the major planets, their composition, structure, origin, and evolution. This book is an attempt at summarizing our present understanding of the atmospheres and ionospheres in the outer solar system, with particular emphasis on the relevant physics and chemistry. I was motivat- ed to prepare this manuscript for the following reasons. First, after under- going rapid expansion in the recent past, the subject has finally attained 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
Pindex Book 1986
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發(fā)表于 2025-3-21 22:00:27 | 只看該作者
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
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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
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發(fā)表于 2025-3-22 17:41:21 | 只看該作者
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
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發(fā)表于 2025-3-23 00:18:55 | 只看該作者
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
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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
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發(fā)表于 2025-3-23 06:12:00 | 只看該作者
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
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