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Convection in the interiors of planets

✍ Scribed by Z.F. Daneš


Publisher
Elsevier Science
Year
1969
Tongue
English
Weight
310 KB
Volume
10
Category
Article
ISSN
0019-1035

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We propose a quasigeostrophic, baroclinic model for heat transport within the interior of a stably stratified Jovian planet, based on motion in thin cylindrical annuli. Density decreases from the center outward and is zero at the surface of the planet. In the homogeneous case (no core), we find inst