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Dawson, D. G.; Patel, M. R. and Lewis, S. R.
(2012).
URL: http://meetingorganizer.copernicus.org/EPSC2012/EP...
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.
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- Item ORO ID
- 35166
- Item Type
- Conference or Workshop Item
- Project Funding Details
-
Funded Project Name Project ID Funding Body Not Set Not Set Science & Technology Facilities Council - Extra Information
-
EPSC Abstracts
Vol. 7 EPSC2012-180 2012 - Keywords
- Mars; atmosphere; UVIS
- 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
- Depositing User
- Daniel Dawson