Jupiter's Great Red Spot: compactness condition and stability

Linear Rossby wave dispersion relationships suggest that Jupiter's Great Red Spot (GRS) is a baroclinic structure embedded in a barotropic shearing zonal flow. Quasi-geostrophic (QG) two-layer simulations support the theory, as long as an infinitely deep zonal flow is assumed. However, once...

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Bibliographic Details
Main Authors: J.-I. Yano, G. R. Flierl
Format: Article
Language:English
Published: Copernicus Publications 1994-01-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/12/1/1994/angeo-12-1-1994.pdf

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