Holmes, J. A.; Lewis, S. R. and Patel, M. R.
(2012).
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| URL: | http://meetingorganizer.copernicus.org/EPSC2012/EP... |
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Abstract
Ozone, water vapour and argon are minor constituents in the Martian atmosphere, observations of which can be of use in constraining atmospheric dynamical and physical processes. This is especially true in the winter season of each hemisphere, when the bulk of the main constituent in the atmosphere (CO2 ) condenses in the polar regions shifting the balance of atmospheric composition to a more trace gas rich air mass. Current Mars Global Circulation Models (MGCMs) are able to represent the photochemistry occuring in the atmosphere, with constraints being imposed by comparisons with observations. However, a long term comparison using data assimilation provides a more robust constraint on the model. We aim to provide a technique for trace gas data assimilation for the analysis of observations from current and future satellite missions (such as ExoMars) which observe the spatial and temporal distribution of trace gases on Mars.
| 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 EPSC2012-217-2 2012 |
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| Keywords: | Mars; data assimilation; trace gases | ||||||
| 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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| Research Group: | Space | ||||||
| Item ID: | 34455 | ||||||
| Depositing User: | James Holmes | ||||||
| Date Deposited: | 17 Oct 2012 12:33 | ||||||
| Last Modified: | 02 May 2018 13:43 | ||||||
| URI: | http://oro.open.ac.uk/id/eprint/34455 | ||||||
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