Mendonça, João M.; Read, Peter L.; Lewis, Stephen R. and Lee, Christopher
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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:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Stephen Lewis|
|Date Deposited:||09 Jul 2012 09:27|
|Last Modified:||05 Oct 2016 03:37|
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