Cloud structure and composition of Jupiter's troposphere from 5-m Cassini VIMS spectroscopy
Jupiter's tropospheric composition and cloud structure are studied using Cassini VIMS 4.5-5.1 m thermal emission spectra from the 2000-2001 flyby. We make use of both nadir and limb darkening observations on the planet's nightside, and compare these with dayside observations. Although ther...
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Published in | Icarus (New York, N.Y. 1962) Vol. 257; pp. 457 - 470 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
01.09.2015
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Subjects | |
Online Access | Get full text |
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