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The new Oxford planetary unified model system for Venus (OPUS-V)

The new Oxford planetary unified model system for Venus (OPUS-V)
The new Oxford planetary unified model system for Venus (OPUS-V)
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.
Lunar and Planetary Institute
Mendonca, J.~M.
cb29fe08-eb94-4fad-8eba-eac1c5de491b
Read, Peter L.
0c70516f-56ef-4f86-91e7-c55f9b49d8ba
Lewis, Stephen R.
c6731362-ff40-4921-81ac-de6ae053589e
Lee, Christopher
f04a8b45-0c48-4678-bf51-95ae42744ed6
Mendonca, J.~M.
cb29fe08-eb94-4fad-8eba-eac1c5de491b
Read, Peter L.
0c70516f-56ef-4f86-91e7-c55f9b49d8ba
Lewis, Stephen R.
c6731362-ff40-4921-81ac-de6ae053589e
Lee, Christopher
f04a8b45-0c48-4678-bf51-95ae42744ed6

Mendonca, J.~M., Read, Peter L., Lewis, Stephen R. and Lee, Christopher (2012) The new Oxford planetary unified model system for Venus (OPUS-V). In Comparative Climatology of Terrestrial Planets. Lunar and Planetary Institute..

Record type: Conference or Workshop Item (Paper)

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.

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More information

Published date: June 2012
Venue - Dates: Comparative Climatology of Terrestrial Planets, , Boulder, United States, 2012-06-25 - 2012-06-28
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Identifiers

Local EPrints ID: 496790
URI: http://eprints.soton.ac.uk/id/eprint/496790
PURE UUID: 35114c64-fce8-4bcc-81aa-5e5358014e93
ORCID for J.~M. Mendonca: ORCID iD orcid.org/0000-0002-6907-4476

Catalogue record

Date deposited: 08 Jan 2025 05:26
Last modified: 10 Jan 2025 03:21

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Contributors

Author: J.~M. Mendonca ORCID iD
Author: Peter L. Read
Author: Stephen R. Lewis
Author: Christopher Lee

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