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dc.contributor.authorMahieux, A.
dc.contributor.authorBerkenbosch, S.
dc.contributor.authorClairquin, R.
dc.contributor.authorFussen, D.
dc.contributor.authorMateshvili, N.
dc.contributor.authorNeefs, E.
dc.contributor.authorNevejans, D.
dc.contributor.authorRistic, B.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorWilquet, V.
dc.contributor.authorBelyaev, D.
dc.contributor.authorFedorova, A.
dc.contributor.authorKorablev, O.
dc.contributor.authorVillard, E.
dc.contributor.authorMontmessin, F.
dc.contributor.authorBertaux, J.-L.
dc.date2008
dc.date.accessioned2016-09-21T12:08:06Z
dc.date.available2016-09-21T12:08:06Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4348
dc.descriptionSolar occultation in the infrared, part of the Spectoscopy for Investigation of Characteristics of the Atmosphere of Venus (SPICAV) instrument onboard Venus Express, combines an echelle grating spectrometer with an acousto-optic tunable filter (AOTF). It performs solar occultation measurements in the IR region at high spectral resolution. The wavelength range probed allows a detailed chemical inventory of Venus's atmosphere above the cloud layer, highlighting the vertical distribution of gases. A general description of the instrument and its in-flight performance is given. Different calibrations and data corrections are investigated, in particular the dark current and thermal background, the nonlinearity and pixel-to-pixel variability of the detector, the sensitivity of the instrument, the AOTF properties, and the spectral calibration and resolution.
dc.languageeng
dc.titleIn-flight performance and calibration of SPICAV SOIR onboard Venus Express
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeGeneral description
dc.subject.freeIn-flight performance
dc.subject.freeVenus Express
dc.subject.freeCalibration
dc.source.titleApplied Optics
dc.source.volume47
dc.source.issue13
dc.source.page2252-2265
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/AO.47.002252
dc.identifier.scopus2-s2.0-50849134875


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