- Abstract:
-
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 equations. The vertical resolution near the surface has been refined, and the vertical domain has been extended to above 80 km. These changes are accompanied by the inclusion of state-of-the-art p...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1029/1999JE001025
-
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- Journal:
- JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
- Volume:
- 104
- Issue:
- E10
- Pages:
- 24155-24175
- Publication date:
- 1999-10-25
- DOI:
- ISSN:
-
0148-0227
- URN:
-
uuid:23ba4973-09a6-4fc3-801e-820917743981
- Source identifiers:
-
21170
- Local pid:
- pubs:21170
- Language:
- English
- Copyright date:
- 1999
Journal article
Improved general circulation models of the Martian atmosphere from the surface to above 80 km
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