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dc.contributor.authorLazar, M.
dc.contributor.authorPierrard, V.
dc.contributor.authorShaaban, S.M.
dc.contributor.authorFichtner, H.
dc.contributor.authorPoedts, S.
dc.date2017
dc.date.accessioned2017-06-09T10:25:59Z
dc.date.available2017-06-09T10:25:59Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5782
dc.languageeng
dc.titleDual Maxwellian-Kappa modeling of the solar wind electrons: new clues on the temperature of Kappa populations
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAstronomy and Astrophysics
dc.source.volume602
dc.source.pageA44
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/0004-6361/201630194


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