Improved general circulation models of the Martian atmosphere from the surface to above 80 km
We describe a set of two “new generation” general circulation models of the Martian atmosphere derived from the models we originally developed in the early 1990s. The two new models share the same physical parameterizations but use two complementary numerical methods to solve the atmospheric dynamic...
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Veröffentlicht in: | Journal of Geophysical Research: Planets 1999-10, Vol.104 (E10), p.24155-24175 |
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Hauptverfasser: | , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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