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A search for the infrared spectroscopic signature of hot Jupiter planets

✍ Scribed by P. W. Lucas; P. F. Roche


Publisher
John Wiley and Sons
Year
2002
Tongue
English
Weight
124 KB
Volume
336
Category
Article
ISSN
0035-8711

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We present a three-dimensional cloud model designed for the study of formation and evolution of moist convective storms on the giant planets. This is a finite-difference model that solves the dynamic and thermodynamic equations forward in time under the anelastic approximation including microphysics