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Bending, V. L.; Lewis, S. R. and Kolb, U.
(2012).
URL: http://meetingorganizer.copernicus.org/EPSC2012/EP...
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.
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- Item ORO ID
- 34429
- Item Type
- Conference or Workshop Item
- Extra Information
-
EPSC Abstracts
Vol. 7 EPSC2012-893 2012
European Planetary Science Congress 2012 - Keywords
- exoplanets; atmospheric modelling
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- ?? space ??
- Copyright Holders
- © 2012 The Authors
- Related URLs
- Depositing User
- Vicky Bending