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Remote sensing of a magnetotail reconnection X-line using polar rain electrons

Alexeev, IV; Sergeev, V; Owen, CJ; Fazakerley, A; Lucek, E; Reme, H; (2006) Remote sensing of a magnetotail reconnection X-line using polar rain electrons. Geophysical Research Letters , 33 (19) , Article L19105. 10.1029/2006GL027243. Green open access

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Abstract

We report on electron phase space distributions (PSDs) observed near the plasma sheet (PS) boundary layer (PSBL) by the Cluster electron spectrometers when the northern lobe was occupied by significant fluxes of polar rain (PR) electrons. These observations reveal the spatial structure of the electron transition layer (TL) between the polar rain electrons and the PSBL electron population accelerated during reconnection. This TL comprises overlapping spatial dispersion signatures in both energy and pitch angle, which are caused by convection of flux tubes across the magnetic separatrix during the electron time-of-flight (TOF) from the X-line combined with acceleration in the reconnection region. Analysis of this structure allows us to estimate the location of the X-line. By assuming the PSBL population arises through acceleration of the PR electrons, comparison of their PSD indicates that the electrons gain energy proportional to their initial energy.

Type: Article
Title: Remote sensing of a magnetotail reconnection X-line using polar rain electrons
Open access status: An open access version is available from UCL Discovery
DOI: 10.1029/2006GL027243
Publisher version: http://dx.doi.org/10.1029/2006GL027243
Language: English
Additional information: Copyright 2006 by the American Geophysical Union
Keywords: Plasma sheet boundary, Cluster
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/157364
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