Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results

On the basis of ARTEMIS two-probe mission magnetic reconnection (MR) outflow associated magnetic fluctuations and turbulence are analyzed on 19 February 2011. In the deep-tail, at distances between <i>X</i> = 45 – 51 <i>R</i>&...

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Main Author: Z. Vörös
Format: Article
Language:English
Published: Copernicus Publications 2011-11-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/18/861/2011/npg-18-861-2011.pdf
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author Z. Vörös
author_facet Z. Vörös
author_sort Z. Vörös
collection DOAJ
description On the basis of ARTEMIS two-probe mission magnetic reconnection (MR) outflow associated magnetic fluctuations and turbulence are analyzed on 19 February 2011. In the deep-tail, at distances between <i>X</i> = 45 – 51 <i>R</i><sub>E</sub>, evidence for reconnection associated plasma sheet thinning was found, accompanied by heating of the plasma sheet. Correlated flow and field reversals and the large-scale Hall-effect signatures indicated the presence of the reconnection <i>X</i>-line. Within fast reconnection plasma outflows, magnetic fluctuations exhibit the same spectral scaling features and kinked spectra as magnetic fluctuations in the solar wind or in various parts of geospace. It was shown that the proton scale magnetic fluctuations are constrained by oblique firehose, proton cyclotron and mirror instability thresholds. For parallel plasma β<sub>||</sub> > 1, where the thresholds converge, perpendicular magnetic fluctuations are enhanced. Magnetic compressibility decreases with the distance to the neutral sheet, however, near the instability thresholds it is comparable to the values obtained in the solar wind.
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spelling doaj.art-38fc4c593fdb47109cc9c5ab2d9ea2292022-12-22T02:04:41ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462011-11-0118686186910.5194/npg-18-861-2011Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS resultsZ. VörösOn the basis of ARTEMIS two-probe mission magnetic reconnection (MR) outflow associated magnetic fluctuations and turbulence are analyzed on 19 February 2011. In the deep-tail, at distances between <i>X</i> = 45 – 51 <i>R</i><sub>E</sub>, evidence for reconnection associated plasma sheet thinning was found, accompanied by heating of the plasma sheet. Correlated flow and field reversals and the large-scale Hall-effect signatures indicated the presence of the reconnection <i>X</i>-line. Within fast reconnection plasma outflows, magnetic fluctuations exhibit the same spectral scaling features and kinked spectra as magnetic fluctuations in the solar wind or in various parts of geospace. It was shown that the proton scale magnetic fluctuations are constrained by oblique firehose, proton cyclotron and mirror instability thresholds. For parallel plasma β<sub>||</sub> > 1, where the thresholds converge, perpendicular magnetic fluctuations are enhanced. Magnetic compressibility decreases with the distance to the neutral sheet, however, near the instability thresholds it is comparable to the values obtained in the solar wind.http://www.nonlin-processes-geophys.net/18/861/2011/npg-18-861-2011.pdf
spellingShingle Z. Vörös
Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
Nonlinear Processes in Geophysics
title Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
title_full Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
title_fullStr Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
title_full_unstemmed Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
title_short Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
title_sort magnetic reconnection associated fluctuations in the deep magnetotail artemis results
url http://www.nonlin-processes-geophys.net/18/861/2011/npg-18-861-2011.pdf
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