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Composition, seasonal change, and bathymetry of Ligeia Mare, Titan, derived from its microwave thermal emission

dc.contributor.authorLe Gall A.
dc.contributor.authorMalaska M. J.
dc.contributor.authorLorenz R. D.
dc.contributor.authorJanssen M. A.
dc.contributor.authorTokano T.
dc.contributor.authorHayes A. G.
dc.contributor.authorMastrogiuseppe M.
dc.contributor.authorLunine J. I.
dc.contributor.authorVeyssière G.
dc.contributor.authorEncrenaz P.
dc.contributor.authorKaratekin O.
dc.date2/2016
dc.date.accessioned2016-04-13T10:08:53Z
dc.date.available2016-04-13T10:08:53Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3968
dc.descriptionhttp://esoads.eso.org/abs/2016JGRE..121..233L
dc.languageeng
dc.rightsRestricted Access
dc.titleComposition, seasonal change, and bathymetry of Ligeia Mare, Titan, derived from its microwave thermal emission
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research (Planets)
dc.source.volume121
dc.source.page233
Orfeo.peerreviewedYes
dc.identifier.doi10.1002/2015JE004920
dc.identifier.urlhttp://esoads.eso.org/abs/2016JGRE..121..233L
dc.source.editorWILEY


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