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dc.contributor.authorVandaele, A.C.
dc.contributor.authorChamberlain, S.
dc.contributor.authorMahieux, A.
dc.contributor.authorRistic, B.
dc.contributor.authorRobert, S.
dc.contributor.authorThomas, I.
dc.contributor.authorTrompet, L.
dc.contributor.authorWilquet, V.
dc.contributor.authorBelyaev, D.
dc.contributor.authorFedorova, A.
dc.contributor.authorKorablev, O.
dc.contributor.authorBertaux, J.L.
dc.contributor.editor
dc.date2016
dc.date.accessioned2016-05-25T11:00:39Z
dc.date.available2016-05-25T11:00:39Z
dc.identifier.urihttps://orfeo.kbr.be/handle/internal/3998
dc.descriptionThe SOIR instrument on-board Venus Express is an infrared spectrometer covering the 2.2-4.3μm spectral region. This instrument allows the detection of several key species of the Venus atmosphere, including CO<inf>2</inf>, CO, H<inf>2</inf>O/HDO, HCl, HF and SO<inf>2</inf>. From the CO<inf>2</inf> density measurements, temperature is inferred giving information on the thermal structure of the atmosphere. Here we described the kind of data (profiles, latitudinal average, etc.) that will be provided to the updated VIRA compilation. © 2015 COSPAR.
dc.languageeng
dc.titleContribution from SOIR/VEX to the updated Venus International Reference Atmosphere (VIRA)
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeSpace research
dc.subject.freeStructure (composition)
dc.subject.freeSolar occultation
dc.subject.freeSpectral region
dc.subject.freeThermal structure
dc.subject.freeTrace-gases
dc.subject.freeVenus
dc.subject.freeVenus atmospheres
dc.subject.freeVenus Express
dc.subject.freeVertical profile
dc.subject.freeAerospace engineering
dc.source.titleAdvances in Space Research
dc.source.volume57
dc.source.page443-458
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.asr.2015.08.012
dc.identifier.scopus2-s2.0-84940703188


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