Show simple item record

dc.contributor.authorGiuranna, M.
dc.contributor.authorTellmann, S.
dc.contributor.authorMontmessin, F.
dc.contributor.authorBelyaev, D.
dc.contributor.authorTrompet, L.
dc.contributor.authorPätzold, M.
dc.contributor.authorWolkenberg, P.
dc.contributor.authorLopez-Valverde, M.A.
dc.contributor.authorKorablev, O.
dc.contributor.authorForget, F.
dc.date2025
dc.date.accessioned2025-04-07T06:54:40Z
dc.date.available2025-04-07T06:54:40Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/14001
dc.descriptionLaunched in 2003, the European Space Agency’s Mars Express (MEX) has been orbiting Mars for 20 years and its instruments have performed continuous monitoring of the conditions in the Martian atmosphere, providing one of the most complete datasets of atmospheric parameters ever collected for Mars. This article provides an overview of the observations of the vertical structure of the Martian atmosphere performed by MEx, which led to the identification of peculiar phenomena that affect the atmospheric circulation and dynamics on different scales, from local to regional and global.
dc.languageeng
dc.titleVertical Structure of the Martian Atmosphere: The View from Mars Express
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSpace Science Reviews
dc.source.volume221
dc.source.issue3
dc.source.pageA36
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11214-025-01155-9
dc.identifier.url


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record