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This project aims to bring together models of both the atmospheric circulation and interior structure and apply them to close-in gas giant exoplanets, with the intent of producing information that can be used to inform and interpret observations. To this end, an atmospheric model has been modified, and an interior model is being adapted. Scans through parameter space are being performed with the atmospheric model to validate the modifications.
|Item Type:||Conference Item|
|Copyright Holders:||2010 The Authors|
|Extra Information:||Poster presentation|
|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:||Vicky Bending|
|Date Deposited:||24 Nov 2010 12:00|
|Last Modified:||05 Oct 2016 03:37|
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