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dc.contributor.authorNeefs, E.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorDrummond, R.
dc.contributor.authorThomas, I.R.
dc.contributor.authorBerkenbosch, S.
dc.contributor.authorClairquin, R.
dc.contributor.authorDelanoye, S.
dc.contributor.authorRistic, B.
dc.contributor.authorMaes, J.
dc.contributor.authorBonnewijn, S.
dc.contributor.authorPieck, G.
dc.contributor.authorEqueter, E.
dc.contributor.authorDepiesse, C.
dc.contributor.authorDaerden, F.
dc.contributor.authorVan Ransbeeck, E.
dc.contributor.authorNevejans, D.
dc.contributor.authorRodriguez-Gomez, J.
dc.contributor.authorLopez-Moreno, J.-J.
dc.contributor.authorSanz, R.
dc.contributor.authorMorales, R.
dc.contributor.authorCandini, G.P.
dc.contributor.authorPastor-Morales, M.C.
dc.contributor.authorDel Moral, B.A.
dc.contributor.authorJeronimo-Zafra, J.-M.
dc.contributor.authorGomez-Lopez, J.M.
dc.contributor.authorAlonso-Rodrigo, G.
dc.contributor.authorPerez-Grande, I.
dc.contributor.authorCubas, J.
dc.contributor.authorGomez-Sanjuan, A.M.
dc.contributor.authorNavarro-Medina, F.
dc.contributor.authorThibert, T.
dc.contributor.authorPatel, M.R.
dc.contributor.authorBellucci, G.
dc.contributor.authorDe Vos, L.
dc.contributor.authorLesschaeve, S.
dc.contributor.authorVan Vooren, N.
dc.contributor.authorMoelans, W.
dc.contributor.authorAballea, L.
dc.contributor.authorGlorieux, S.
dc.contributor.authorBaeke, A.
dc.contributor.authorKendall, D.
dc.contributor.authorDe Neef, J.
dc.contributor.authorSoenen, A.
dc.contributor.authorPuech, P.-Y.
dc.contributor.authorWard, J.
dc.contributor.authorJamoye, J.-F.
dc.contributor.authorDiez, D.
dc.contributor.authorVicario-Arroyo, A.
dc.contributor.authorJankowski, M.
dc.date2015
dc.date.accessioned2016-03-24T10:27:12Z
dc.date.available2016-03-24T10:27:12Z
dc.identifier.urihttps://orfeo.kbr.be/handle/internal/2718
dc.descriptionNOMAD is a spectrometer suite on board ESA’s ExoMars trace gas orbiter due for launch in January 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 dayside and nightside, and during solar occultations. In this paper, the design, manufacturing, and testing of the two infrared channels are described. We focus upon the optical working principle in these channels, where an echelle grating, used as a diffractive element, is combined with an acousto-optical tunable filter, used as a diffraction order sorter.
dc.languageeng
dc.titleNOMAD spectrometer on the ExoMars trace gas orbiter mission: Part 1 - design, manufacturing and testing of the infrared channels
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleApplied Optics
dc.source.volume54
dc.source.issue28
dc.source.page8494-8520
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/AO.54.008494


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