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...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
1994-01-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/12/1/1994/angeo-12-1-1994.pdf |