Steele, Liam; Lewis, S. R.; Patel, M. R. and Smith, M. D.
(2012).
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| URL: | http://meetingorganizer.copernicus.org/EPSC2012/EP... |
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Abstract
Water ice clouds have been shown to alter the thermal structure of the Martian atmosphere. Here we discuss the assimilation of total column water vapour and dust optical depth data from the Thermal Emission Spectrometer (TES) into the UK/LMD MGCM, and compare the predictions of cloud and temperature in the assimilation with observations.
| Item Type: | Conference or Workshop Item | ||||||
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| Copyright Holders: | 2012 The Authors | ||||||
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| Extra Information: | EPSC Abstracts
Vol. 7 EPSC2012-321 2012 European Planetary Science Congress 2012 |
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| Keywords: | mars atmosphere water cycle data assimilation | ||||||
| Academic Unit/School: | Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences Faculty of Science, Technology, Engineering and Mathematics (STEM) |
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| Interdisciplinary Research Centre: | Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR) | ||||||
| Item ID: | 35179 | ||||||
| Depositing User: | Liam Steele | ||||||
| Date Deposited: | 07 Nov 2012 10:18 | ||||||
| Last Modified: | 15 May 2017 17:07 | ||||||
| URI: | http://oro.open.ac.uk/id/eprint/35179 | ||||||
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