Linear baroclinic instability in the Martian atmosphere
A spherical quasi-geostrophic model is used in an examination of linear baroclinic instability in such zonal-mean flows as those of the Martian atmosphere in winter, under both relatively nondusty and very dusty conditions. These zonal flows, which possess both vertical and meridional shear, are cha...
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Veröffentlicht in: | Journal of the atmospheric sciences 1984-05, Vol.41 (9), p.1536-1550 |
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Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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