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Theoretical Plasma Distributions Consistent with Ulysses Magnetic Field Observations in a Solar Wind Tangential Discontinuity

dc.contributor.authorDe Keyser, J.
dc.contributor.authorRoth, M.
dc.contributor.authorLemaire, J.
dc.contributor.authorTsurutani, B.T.
dc.contributor.authorHo, C.M.
dc.contributor.authorHammond, C.M.
dc.date1996
dc.date.accessioned2018-03-01T11:06:54Z
dc.date.available2018-03-01T11:06:54Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/6838
dc.languageeng
dc.titleTheoretical Plasma Distributions Consistent with Ulysses Magnetic Field Observations in a Solar Wind Tangential Discontinuity
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAeronomica Acta
dc.source.issue395
Orfeo.peerreviewedNo
dc.identifier.doi10.18758/A_395


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