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dc.contributor.authorPatel, M.R.
dc.contributor.authorAntoine, P.
dc.contributor.authorMason, J.
dc.contributor.authorLeese, M.
dc.contributor.authorHathi, B.
dc.contributor.authorStevens, A.H.
dc.contributor.authorDawson, D.
dc.contributor.authorGow, J.
dc.contributor.authorRingrose, T.
dc.contributor.authorHolmes, J.
dc.contributor.authorLewis, S.R.
dc.contributor.authorBeghuin, D.
dc.contributor.authorVan Donink, P.
dc.contributor.authorLigot, R.
dc.contributor.authorDewandel, J.-L.
dc.contributor.authorHu, D.
dc.contributor.authorBates, D.
dc.contributor.authorCole, R.
dc.contributor.authorDrummond, R.
dc.contributor.authorThomas, I.R.
dc.contributor.authorDepiesse, C.
dc.contributor.authorNeefs, E.
dc.contributor.authorEqueter, E.
dc.contributor.authorRistic, B.
dc.contributor.authorBerkenbosch, S.
dc.contributor.authorBolsée, D.
dc.contributor.authorWillame, Y.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorLesschaeve, S.
dc.contributor.authorDe Vos, L.
dc.contributor.authorVan Vooren, N.
dc.contributor.authorThibert, T.
dc.contributor.authorMazy, E.
dc.contributor.authorRodriguez-Gomez, J.
dc.contributor.authorMorales, R.
dc.contributor.authorCandini, G.P.
dc.contributor.authorPastor-Morales, M.C.
dc.contributor.authorSanz, R.
dc.contributor.authorAparicio del Moral, B.
dc.contributor.authorJeronimo-Zafra, J.-M.
dc.contributor.authorGómez-López, J.M.
dc.contributor.authorAlonso-Rodrigo, G.
dc.contributor.authorPérez-Grande, I.
dc.contributor.authorCubas, J.
dc.contributor.authorGomez-Sanjuan, A.M.
dc.contributor.authorNavarro-Medina, F.
dc.contributor.authorBenmoussa, A.
dc.contributor.authorGiordanengo, B.
dc.contributor.authorGissot, S.
dc.contributor.authorBellucci, G.
dc.contributor.authorLopez-Moreno, J.J.
dc.contributor.editor
dc.date2017
dc.date.accessioned2017-04-18T09:00:23Z
dc.date.available2017-04-18T09:00:23Z
dc.identifier.urihttps://orfeo.kbr.be/handle/internal/5052
dc.descriptionNOMAD is a spectrometer suite on board the ESA/Roscosmos ExoMars Trace Gas Orbiter, which launched in March 2016. NOMAD consists of two infrared channels and one ultraviolet and visible channel, allowing the instrument to perform observations quasi-constantly, by taking nadir measurements at the day-and night-side, and during solar occultations. Here, in part 2 of a linked study, we describe the design, manufacturing, and testing of the ultraviolet and visible spectrometer channel called UVIS. We focus upon the optical design and working principle where two telescopes are coupled to a single grating spectrometer using a selector mechanism.
dc.languageeng
dc.titleNOMAD spectrometer on the ExoMars trace gas orbiter mission: Part 2-design, manufacturing, and testing of the ultraviolet and visible channel
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeManufacture
dc.subject.freeOptical design
dc.subject.freeExoMars
dc.subject.freeInfrared channel
dc.subject.freeNadir measurements
dc.subject.freeSingle grating spectrometer
dc.subject.freeSolar occultation
dc.subject.freeTrace gas
dc.subject.freeVisible channels
dc.subject.freeVisible spectrometers
dc.subject.freeSpectrometers
dc.source.titleApplied Optics
dc.source.volume56
dc.source.issue10
dc.source.page2771-2782
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/AO.56.002771
dc.identifier.scopus2-s2.0-85016791766


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