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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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

pineal-gland

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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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

Mercurial

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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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