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Preliminary characterization of the upper haze by SPICAV/SOIR solar occultation in UV to mid-IR onboard Venus Express

dc.contributor.authorWilquet, V.
dc.contributor.authorFedorova, A.
dc.contributor.authorMontmessin, F.
dc.contributor.authorDrummond, R.
dc.contributor.authorMahieux, A.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorVillard, E.
dc.contributor.authorKorablev, O.
dc.contributor.authorBertaux, J.-L.
dc.date2009
dc.date.accessioned2016-04-05T13:14:13Z
dc.date.available2016-04-05T13:14:13Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3292
dc.languageeng
dc.titlePreliminary characterization of the upper haze by SPICAV/SOIR solar occultation in UV to mid-IR onboard Venus Express
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research E: Planets
dc.source.volume114
dc.source.issue9
dc.source.pageE00B42
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2008JE003186


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