A numerical model of the atmosphere of Venus
A new general circulation model (GCM) of Venus is being developed at Oxford. Venus presents unique numerical and physical challenges because of its thick atmosphere, slow underlying solid body rotation, and super-rotating atmosphere. Preliminary results from a GCM with simplified physical parameteri...
| Auteurs principaux: | , , |
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| Format: | Conference item |
| Publié: |
2005
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