Mendonça, João M.; Read, Peter L.; Lewis, Stephen R. and Lee, Christopher
(2012).
|
PDF (Version of Record)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (56Kb) |
| URL: | http://www.lpi.usra.edu/meetings/climatology2012/p... |
|---|---|
| Google Scholar: | Look up in Google Scholar |
Abstract
We present a new version of the Oxford Venus GCM, which using our new parameterisations produce a realistic Venus mesosphere atmospheric circulation. We present results that give hints to the formation of global super-rotation.
| Item Type: | Conference Item |
|---|---|
| Copyright Holders: | 2012 The Authors |
| Academic Unit/Department: | Science > Physical Sciences |
| Interdisciplinary Research Centre: | Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR) |
| Related URLs: | |
| Item ID: | 33961 |
| Depositing User: | Stephen Lewis |
| Date Deposited: | 09 Jul 2012 09:27 |
| Last Modified: | 17 Nov 2012 11:10 |
| URI: | http://oro.open.ac.uk/id/eprint/33961 |
Actions (login may be required)
| View Item | |
| Public: Report issue / request change |




