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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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| Main Authors: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Copernicus Publications
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| Colecção: | Annales Geophysicae |
| Acesso em linha: | http://www.ann-geophys.net/12/1/1994/angeo-12-1-1994.html |
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