Bending, V. L.; Lewis, S. R. and Kolb, U.
(2012).
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| URL: | http://meetingorganizer.copernicus.org/EPSC2012/EP... |
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Abstract
Many models are used to study the possible atmospheric conditions of extrasolar gas giants, in particular “hot Jupiters”, gas giant planets closer than 0.1 AU to their parent stars, with orbital periods of the order of a few Earth days. It is important that the respective responses of these models to this relatively new regime be known, allowing the effects of using different models to be understood. Here, the use of an adapted form of the PUMA model is explored by carrying out an intercomparison test.
| Item Type: | Conference Item |
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| Copyright Holders: | 2012 The Authors |
| Extra Information: | EPSC Abstracts
Vol. 7 EPSC2012-893 2012 European Planetary Science Congress 2012 |
| Keywords: | exoplanets; atmospheric modelling |
| Academic Unit/Department: | Science > Physical Sciences |
| Interdisciplinary Research Centre: | Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR) |
| Related URLs: | |
| Item ID: | 34429 |
| Depositing User: | Vicky Bending |
| Date Deposited: | 02 Oct 2012 08:49 |
| Last Modified: | 27 Feb 2013 17:41 |
| URI: | http://oro.open.ac.uk/id/eprint/34429 |
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