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Robert, S.; Vandaele, A.C.; Thomas, I.; Willame, Y.; Daerden, F.; Delanoye, S.; Depiesse, C.; Drummond, R.; Neefs, E.; Neary, L.; Ristic, B.; Mason, J.; Lopez-Moreno, J.-J.; Rodriguez-Gomez, J.; Patel, M. R.; Bellucci, G. and The NOMAD Team, .
(2016).
DOI: https://doi.org/10.1016/j.pss.2016.03.003
Abstract
NOMAD (Nadir and Occultation for MArs Discovery) is one of the four instruments on board the ExoMars Trace Gas Orbiter, scheduled for launch in March 2016. It consists of a suite of three high-resolution spectrometers – SO (Solar Occultation), LNO (Limb, Nadir and Occultation) and UVIS (Ultraviolet and Visible Spectrometer). Based upon the characteristics of the channels and the values of Signal-to-Noise Ratio obtained from radiometric models discussed in [Vandaele et al., Optics Express, 2015] and [Thomas et al., Optics Express, 2015], the expected performances of the instrument in terms of sensitivity to detection have been investigated. The analysis led to the determination of detection limits for 18 molecules, namely CO, H2O, HDO, C2H2, C2H4, C2H6, H2CO, CH4, SO2, H2S, HCl, HCN, HO2, NH3, N2O, NO2, OCS, O3. NOMAD should have the ability to measure methane concentrations <25 parts per trillion (ppt) in solar occultation mode, and 11 parts per billion in nadir mode. Occultation detections as low as 10 ppt could be made if spectra are averaged [Drummond et al., Planetary Space and Science, 2011]. Results have been obtained for all three channels in nadir and in solar occultation.
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About
- Item ORO ID
- 45619
- Item Type
- Journal Item
- ISSN
- 0032-0633
- Project Funding Details
-
Funded Project Name Project ID Funding Body NOMAD Not Set BELSPO NOMAD Not Set ESA Prodex Office Interuniversity Attraction Poles Not Set Planet TOPERS Interuniversity Attraction Poles BR/143/A2/SCOOP BRAIN Seventh Framework Programme FP7/2007-2013 European Community Not Set ST/I003061/1 UK Space Agency - Keywords
- ExoMars ESA mission; NOMAD instrument; Mars; atmosphere; Abundances; Radiative transfer
- Academic Unit or School
- Other Departments > Other Departments
- Copyright Holders
- © 2016 Elsevier
- Depositing User
- Manish Patel