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dc.contributor.authorMahieux, A.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorRobert, S.
dc.contributor.authorWilquet, V.
dc.contributor.authorDrummond, R.
dc.contributor.authorMontmessin, F.
dc.contributor.authorBertaux, J.L.
dc.date2012
dc.date.accessioned2016-03-29T10:07:35Z
dc.date.available2016-03-29T10:07:35Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2967
dc.descriptionSOIR is a high-resolution spectrometer flying on board the ESA Venus Express mission. It performs solar occultations of the Venus high atmosphere, and so defines unique vertical profiles of many of the Venus key species. In this paper, we focus on the Venus main constituent, carbon dioxide. We explain how the temperature, the total density, and the total pressure are derived from the observed CO 2 density vertical profiles. A striking permanent temperature minimum at 125 km is observed. The data set is processed in order to obtain a Venus Atmosphere from SOIR measurements at the Terminator (VAST) compilation for different latitude regions and extending from 70 up to 170 km in altitude. The results are compared to many literature results obtained from ground-based observations, previous missions, and the Venus Express mission. The homopause altitude is also determined.
dc.languageeng
dc.titleDensities and temperatures in the Venus mesosphere and lower thermosphere retrieved from SOIR on board Venus Express: Carbon dioxide measurements at the Venus terminator
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeair temperature
dc.subject.freecarbon dioxide
dc.subject.freemesosphere
dc.subject.freeplanetary atmosphere
dc.subject.freesatellite imagery
dc.subject.freethermosphere
dc.subject.freeVenus
dc.source.titleJournal of Geophysical Research E: Planets
dc.source.volume117
dc.source.issue7
dc.source.pageE07001
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2012JE004058
dc.identifier.scopus2-s2.0-84863468204


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