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Radiative transfer modelling for the NOMAD-UVIS instrument on the ExoMars Trace Gas Orbiter mission

Dawson, D. G.; Patel, M. R.; Lewis, S. R.; Mason, J. P. and Irwin, P. G. J. (2013). Radiative transfer modelling for the NOMAD-UVIS instrument on the ExoMars Trace Gas Orbiter mission. In: European Planetary Science Congress, 9-13 Sep 2013, London, European Planetary Science Congress.

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Abstract

The NOMAD (Nadir and Occultation for MArs Discovery) instrument is a 3-channel (2 IR, 1 UV/Vis) spectrometer due to fly on the 2016 ExoMars Trace Gas Orbiter mission. A radiative transfer model for Mars has been developed providing synthetic spectra to simulate observations of the UVIS channel in both solar occultation and nadir viewing geometries. This will allow for the characterization and mitigation of the influence of dust on retrievals of ozone abundance.

Item Type: Conference or Workshop Item
Copyright Holders: 2013 The Authors
Project Funding Details:
Funded Project NameProject IDFunding Body
Not SetNot SetSTFC (Science & Technology Facilities Council)
Extra Information: EPSC Abstracts
Vol. 8, EPSC2013-376, 2013
European Planetary Science Congress 2013
Keywords: Mars; NOMAD; UVIS; ExoMars; Radiative Transfer; Ozone; Dust
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Research Group: Space
Item ID: 38568
Depositing User: Daniel Dawson
Date Deposited: 25 Sep 2013 14:06
Last Modified: 09 Dec 2018 13:35
URI: http://oro.open.ac.uk/id/eprint/38568
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