Dawson, D. G.; Patel, M. R. and Lewis, S. R.
(2012).
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| URL: | http://meetingorganizer.copernicus.org/EPSC2012/EP... |
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Abstract
The Ultraviolet and Visible Spectrometer (UVIS) instrument development process requires the construction of an atmospheric model to provide synthetic UV transmission spectra. We discuss the requirements of the model to enable observational limits to be found, and the potential for certain atmospheric parameters to be further constrained.
| Item Type: | Conference Item | ||||||
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| Copyright Holders: | 2012 The Authors | ||||||
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| Extra Information: | EPSC Abstracts
Vol. 7 EPSC2012-180 2012 |
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| Keywords: | Mars; atmosphere; UVIS | ||||||
| Academic Unit/Department: | Science > Physical Sciences | ||||||
| Interdisciplinary Research Centre: | Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR) | ||||||
| Item ID: | 35166 | ||||||
| Depositing User: | Daniel Dawson | ||||||
| Date Deposited: | 07 Nov 2012 09:57 | ||||||
| Last Modified: | 07 Nov 2012 09:57 | ||||||
| URI: | http://oro.open.ac.uk/id/eprint/35166 | ||||||
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