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...
| Autor principal: | |
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| Outros Autores: | , , , , |
| Formato: | lecture |
| Idioma: | eng |
| Publicado em: |
2012
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| Assuntos: | |
| Texto completo: | http://hdl.handle.net/10174/6911 |
| País: | Portugal |
| Oai: | oai:dspace.uevora.pt:10174/6911 |