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Non-equilibrium radiative processes in the atmospheres of the giant planets

✍ Scribed by Robert A. Stokes; Wendell C. Demarcus


Book ID
116042991
Publisher
Elsevier Science
Year
1971
Tongue
English
Weight
463 KB
Volume
4
Category
Article
ISSN
0031-9201

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Fast rotating giant planets such as Jupiter and Saturn possess alternate prograde and retrograde zonal winds which are stable over long periods of time. We consider a compressible model of convection in a spherical shell with rapid rotation, using the anelastic approximation, to explore the paramete