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Venus's winds and temperatures during the MESSENGER's flyby: An approximation to a three-dimensional instantaneous state of the atmosphere

dc.contributor.authorPeralta, J.
dc.contributor.authorLee, Y.J.
dc.contributor.authorHueso, R.
dc.contributor.authorClancy, R.T.
dc.contributor.authorSandor, B.J.
dc.contributor.authorSánchez-Lavega, A.
dc.contributor.authorLellouch, E.
dc.contributor.authorRengel, M.
dc.contributor.authorMachado, P.
dc.contributor.authorOmino, M.
dc.contributor.authorPiccialli, A.
dc.contributor.authorImamura, T.
dc.contributor.authorHorinouchi, T.
dc.contributor.authorMurakami, S.
dc.contributor.authorOgohara, K.
dc.contributor.authorLuz, D.
dc.contributor.authorPeach, D.
dc.date2017
dc.date.accessioned2017-05-29T08:49:04Z
dc.date.available2017-05-29T08:49:04Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5555
dc.languageeng
dc.titleVenus's winds and temperatures during the MESSENGER's flyby: An approximation to a three-dimensional instantaneous state of the atmosphere
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleGeophysical Research Letters
dc.source.volume44
dc.source.issue8
dc.source.page3907-3915
Orfeo.peerreviewedYes
dc.identifier.doi10.1002/2017GL072900


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