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dc.contributor.authorVandaele, A.C.
dc.contributor.authorKorablev, O.
dc.contributor.authorBelyaev, D.
dc.contributor.authorChamberlain, S.
dc.contributor.authorEvdokimova, D.
dc.contributor.authorEncrenaz, T.
dc.contributor.authorEsposito, L.
dc.contributor.authorJessup, K.L.
dc.contributor.authorLefèvre, F.
dc.contributor.authorLimaye, S.
dc.contributor.authorMahieux, A.
dc.contributor.authorMarcq, E.
dc.contributor.authorMills, F.B.
dc.contributor.authorMontmessin, F.
dc.contributor.authorParkinson, C.D.
dc.contributor.authorRobert, S.
dc.contributor.authorRoman, T.
dc.contributor.authorSandor, B.
dc.contributor.authorStolzenbach, A.
dc.contributor.authorWilson, C.
dc.contributor.authorWilquet, V.
dc.contributor.editor
dc.date2017
dc.date.accessioned2017-05-29T08:49:04Z
dc.date.available2017-05-29T08:49:04Z
dc.identifier.urihttps://orfeo.kbr.be/handle/internal/5556
dc.languageeng
dc.titleSulfur dioxide in the Venus atmosphere: I. Vertical distribution and variability
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleIcarus
dc.source.volume295
dc.source.page16-33
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.icarus.2017.05.003


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