Winds and cloud morphology in the southern polar region of Venus
Spinning on average 60 times faster than the surface, the atmosphere of Venus is superrotational, a state in which the averaged angular momentum is much greater than that corresponding to co-rotation with the solid globe. The rapid mean flow, which is main- tained by momentum transports in the deep...
Main Authors: | , , , , , |
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Format: | Lecture |
Language: | English |
Published: |
European Planetary Science Congress 2010
2010
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Subjects: | |
Online Access: | http://hdl.handle.net/10174/6911 http://meetings.copernicus.org/epsc2010/abstracts/EPSC2010-670.pdf |