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In situ evidence of a near-Earth X-line at~11R_E

P.C.Brandt  C.M.Carr  H.Réme  I.Dandouras  
【摘要】:正Magnetic reconnection in the geomagnetotail,responsible for many magnetospheric dynamic behaviors,is widely believed to occur beyond 15 R_E tailward.Therefore in current theoretical models,most near-Earth magnetospheric activities,such as auroras,substorms and geomagnetic storms,are thought not directly to be triggered by tail reconnection.Certain intermediate processes then have to be assumed.Here

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