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dc.contributor.authorEchim, M.
dc.contributor.authorLamy, H.
dc.contributor.authorSimon-Wedlund, C.
dc.contributor.authorDe Keyser, J.
dc.contributor.authorCessateur, G.
dc.date2023
dc.date.accessioned2023-12-16T12:42:09Z
dc.date.available2023-12-16T12:42:09Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/11220
dc.descriptionObservations of a quiet electrostatic auroral arc by the ALIS network on 5 March 2008 are used to infer a two-dimensional map of the flux of precipitating energy. Among a family of numerical solutions of a stationary magnetosphere—ionosphere coupling model in which the origin of the arc is a magnetospheric generator interface, we find which generator interface properties best fit the observed precipitating energy flux. The procedure finds that the plasma populations in the generator are colder and more rarefied on one side of the interface and warmer and denser on the other side, similar to a transition between plasma trough and plasma sheet plasmas. The increase of the arc's brightness, the decrease of its thickness and its slight spatial undulation may be driven by an increase of plasma sheet electron temperature in the tailward direction, tangential to the interface, and a local spatial indentation in the dawn-ward direction.
dc.languageeng
dc.titleProbing the Magnetospheric Generator of Quiet Electrostatic Auroral Arcs From Ground Based Optical Observations and Magnetosphere-ionosphere Coupling Modeling
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freequiet electrostatic auroral arc
dc.subject.freemagnetosphere-ionosphere coupling
dc.subject.freemagnetospheric generator
dc.source.titleGeophysical Research Letters
dc.source.volume50
dc.source.issue24
dc.source.pagee2023GL103689
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2023GL103689
dc.identifier.url


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