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dc.contributor.authorFear, R.C.
dc.contributor.authorMilan, S.E.
dc.contributor.authorMaggiolo, R.
dc.contributor.authorFazakerley, A.N.
dc.contributor.authorDouras, I.
dc.contributor.authorMende, S.B.
dc.date2014
dc.date.accessioned2016-03-25T09:42:11Z
dc.date.available2016-03-25T09:42:11Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2853
dc.descriptionThe structure of Earth's magnetosphere is poorly understood when the interplanetary magnetic field is northward. Under this condition, uncharacteristically energetic plasma is observed in the magnetotail lobes, which is not expected in the textbook model of the magnetosphere. Using satellite observations, we show that these lobe plasma signatures occur on high-latitude magnetic field lines that have been closed by the fundamental plasma process of magnetic reconnection. Previously, it has been suggested that closed flux can become trapped in the lobe and that this plasma-trapping process could explain another poorly understood phenomenon: the presence of auroras at extremely high latitudes, called transpolar arcs. Observations of the aurora at the same time as the lobe plasma signatures reveal the presence of a transpolar arc. The excellent correspondence between the transpolar arc and the trapped closed flux at high altitudes provides very strong evidence of the trapping mechanism as the cause of transpolar arcs.
dc.languageeng
dc.titleDirect observation of closed magnetic flux trapped in the high-latitude magnetosphere
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeaurora
dc.subject.freelatitude
dc.subject.freemagnetic field
dc.subject.freemagnetosphere
dc.subject.freemagnetotail
dc.subject.freeplasma
dc.subject.freesatellite imagery
dc.source.titleScience
dc.source.volume346
dc.source.issue6216
dc.source.page1506-1510
Orfeo.peerreviewedYes
dc.identifier.doi10.1126/science.1257377
dc.identifier.scopus2-s2.0-84919458999


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