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dc.contributor.authorLabrosse N.
dc.contributor.authorHeinzel P.
dc.contributor.authorVial J.-C.
dc.contributor.authorKucera T.
dc.contributor.authorParenti S.
dc.contributor.authorGunár S.
dc.contributor.authorSchmieder B.
dc.contributor.authorKilper G.
dc.date4/2010
dc.date.accessioned2016-04-13T10:04:32Z
dc.date.available2016-04-13T10:04:32Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3671
dc.descriptionhttp://esoads.eso.org/abs/2010SSRv..151..243L
dc.languageeng
dc.rightsRestricted Access
dc.titlePhysics of Solar Prominences: I—Spectral Diagnostics and Non-LTE Modelling
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSpace Science Reviews
dc.source.volume151
dc.source.page243
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11214-010-9630-6
dc.identifier.urlhttp://esoads.eso.org/abs/2010SSRv..151..243L
dc.source.editorSPRINGER


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