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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.