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dc.contributor.authorDe Keyser, J.
dc.contributor.authorMaggiolo, R.
dc.contributor.authorEchim, M.
dc.contributor.authorDandouras, I.
dc.date2011
dc.date.accessioned2016-03-29T12:43:51Z
dc.date.available2016-03-29T12:43:51Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3067
dc.descriptionThis paper reports Cluster high-altitude observations above the acceleration region of a typical monopolar electric field event at the plasma sheet boundary. The observations reveal both characteristics of waves and signatures of electrostatic acceleration. The observations can be interpreted in terms of low-frequency transverse magnetic waves on the auroral interface. A reconstruction of the spatial structure across the interface, effectively correcting for the slow oscillations of the interface, allows a proper determination of the electric potential and of the upward and downward currents. Because of the long wave period, the auroral system can be understood in terms of a quasi-electrostatic model. In this model, the precipitating plasma sheet particles induce a perpendicular heating of cold ionospheric H+ and O+ ions. As these ions escape from the ionosphere, their perpendicular motion is converted into parallel motion in the divergent geomagnetic field as a result of the conservation of magnetic moment. These ions acquire an additional parallel energy through acceleration by the magnetic-field-aligned electric field in the auroral acceleration region. They also may gain substantial perpendicular energy due to the perpendicular electric field, as the equation image × equation image drift increases with altitude. Both types of acceleration are typical electrostatic phenomena.
dc.languageeng
dc.titleWave signatures and electrostatic phenomena above aurora: Cluster observations and modeling
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research: Space Physics
dc.source.volume116
dc.source.issue6
dc.source.pageA06224
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2010JA016004
dc.identifier.scopus2-s2.0-79960123203


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