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dc.contributor.authorEchim, M.M.
dc.contributor.authorRoth, M.
dc.contributor.authorDe Keyser, J.
dc.date2007
dc.date.accessioned2016-09-26T12:14:18Z
dc.date.available2016-09-26T12:14:18Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4368
dc.descriptionWe consider sheared flows in magnetospheric boundary layers of tangential discontinuity type, forming a structure that is embedded in a large-scale convergent perpendicular electric field. We construct a kinetic model that couples the magnetospheric structure with the topside ionosphere. The contribution of magnetospheric electrons and ionospheric electrons and ions is taken into account into the current-voltage relationship derived for an electric potential monotonically decreasing with the altitude. The solution of the current continuity equation gives the distribution of the ionospheric potential consistent with the given magnetospheric electric potential. The model shows that a sheared magnetospheric flow generates current sheets corresponding to upward field-aligned currents, field-aligned potential drops and narrow bands of precipitating energy, as in discrete auroral arcs. Higher velocity magnetospheric sheared flows have the tendency to produce brighter and slightly broader arcs. An increase in arc luminosity is also associated with enhancements of magnetospheric plasma density, in which case the structures are narrower. Finally, the model predicts that an increase of the electron temperature of the magnetospheric flowing plasma corresponds to slightly wider arcs but does not modify their luminosity.
dc.languageeng
dc.relation.ispartofseries
dc.titleSheared magnetospheric plasma flows and discrete auroral arcs: A quasi-static coupling model
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeaurora
dc.subject.freecoupling
dc.subject.freeelectric field
dc.subject.freeelectron
dc.subject.freeionosphere
dc.subject.freemagnetosphere
dc.subject.freeplasma
dc.source.titleAnnales Geophysicae
dc.source.volume25
dc.source.issue1
dc.source.page317-330
Orfeo.peerreviewedYes
dc.identifier.doi10.5194/angeo-25-1011-2007
dc.identifier.scopus2-s2.0-33846880459


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