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dc.contributor.authorDe Keyser, J.
dc.contributor.authorEchim, M.
dc.date2013
dc.date.accessioned2016-03-25T11:11:11Z
dc.date.available2016-03-25T11:11:11Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2922
dc.descriptionStrong localized high-altitude auroral electric fields, such as those observed by Cluster, are often associated with magnetospheric interfaces. The type of high-altitude electric field profile (monopolar, bipolar, or more complicated) depends on the properties of the plasmas on either side of the interface, as well as on the total electric potential difference across the structure. The present paper explores the role of this cross-field electric potential difference in the situation where the interface is a tangential discontinuity. A self-consistent Vlasov description is used to determine the equilibrium configuration for different values of the transverse potential difference. A major observation is that there exist limits to the potential difference, beyond which no equilibrium configuration of the interface can be sustained. It is further demonstrated how the plasma densities and temperatures affect the type of electric field profile in the transition, with monopolar electric fields appearing primarily when the temperature contrast is large. These findings strongly support the observed association of monopolar fields with the plasma sheet boundary. The role of shear flow tangent to the interface is also examined.
dc.languageeng
dc.titleElectric potential differences across auroral generator interfaces
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeaurora
dc.subject.freedensity
dc.subject.freeelectric field
dc.subject.freemagnetosphere
dc.subject.freeplasma
dc.subject.freeshear flow
dc.subject.freetemperature
dc.source.titleAnnales Geophysicae
dc.source.volume31
dc.source.issue2
dc.source.page251-261
Orfeo.peerreviewedYes
dc.identifier.doi10.5194/angeo-31-251-2013
dc.identifier.scopus2-s2.0-84874353191


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