๐”– Bobbio Scriptorium
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A numerical model comparison of baroclinic instability in the presence of topography

โœ Scribed by Catherine Griffiths; Motoyoshi Ikeda; Peter C. Smith


Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
612 KB
Volume
52
Category
Article
ISSN
0280-6495

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๐Ÿ“œ SIMILAR VOLUMES


Baroclinic Instability in the Interiors
โœ Richard Holme; Andrew P. Ingersoll ๐Ÿ“‚ Article ๐Ÿ“… 1994 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 767 KB

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