Dawson, D. G.; Patel, M. R. and Lewis, S. R.
(2012).
|
PDF (Version of Record)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (2165Kb) | Preview |
| URL: | http://meetingorganizer.copernicus.org/EPSC2012/EP... |
|---|---|
| Google Scholar: | Look up in Google Scholar |
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 | ||||||
|---|---|---|---|---|---|---|---|
| Copyright Holders: | 2012 The Authors | ||||||
| Project Funding Details: |
|
||||||
| Extra Information: | EPSC Abstracts
Vol. 7 EPSC2012-180 2012 |
||||||
| Keywords: | Mars; atmosphere; UVIS | ||||||
| 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) | ||||||
| Item ID: | 35166 | ||||||
| Depositing User: | Daniel Dawson | ||||||
| Date Deposited: | 07 Nov 2012 09:57 | ||||||
| Last Modified: | 02 Aug 2016 16:34 | ||||||
| URI: | http://oro.open.ac.uk/id/eprint/35166 | ||||||
| Share this page: |     |
Download history for this item
These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.