Electrodynamics in a very thin current sheet leading to magnetic reconnection

We study the formation of a very thin current sheet (CS) and associated plasma electrodynamics using three-dimensional (3-D) particle-in-cell simulations with ion to electron mass ratio M/m=1836. The CS is driven by imposed anti-parallel magnetic fields. The noteworthy features of the temporal evolu...

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Main Authors: N. Singh, C. Deverapalli, G. Khazanov
Format: Article
Language:English
Published: Copernicus Publications 2006-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/13/509/2006/npg-13-509-2006.pdf
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spelling doaj-c4aeed70261c4081907a229851dcc5592020-11-25T01:59:41ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462006-01-01135509523Electrodynamics in a very thin current sheet leading to magnetic reconnectionN. SinghN. SinghC. DeverapalliG. KhazanovWe study the formation of a very thin current sheet (CS) and associated plasma electrodynamics using three-dimensional (3-D) particle-in-cell simulations with ion to electron mass ratio M/m=1836. The CS is driven by imposed anti-parallel magnetic fields. The noteworthy features of the temporal evolution of the CS are the following: (i) Steepening of the magnetic field profile B<sub>x</sub>(z) in the central part of the CS, (ii) Generation of three-peak current distribution with the largest peak in the CS center as B<sub>x</sub>(z) steepens, (iii) Generation of converging electric fields forming a potential well in the CS center in which ions are accelerated. (iv) Electron and ion heating in the central part of the CS by current-driven instabilities (CDI). (v) Re-broadening of the CS due to increased kinetic plasma pressure in the CS center. (vi) Generation of electron temperature anisotropy with temperature perpendicular to the magnetic field being larger than the parallel one. (vii) Current disruption by electron trapping in an explosively growing electrostatic instability (EGEI) and electron tearing instability (ETI). (viii)The onset of EGEI coincides with an increase in the electron temperature above the temperature of the initially hot ions as well as the appearance of new shear in the electron drift velocity. (ix) Bifurcation of the central CS by the current disruption. (x) Magnetic reconnection (MR) beginning near the null in B<sub>x</sub> and spreading outward. (xi) Generation of highly energized electrons reaching relativistic speeds and having isotropic pitch-angle distribution in the region of reconnected magnetic fields. We compare some of these features of the current sheet with results from laboratory and space experiments.http://www.nonlin-processes-geophys.net/13/509/2006/npg-13-509-2006.pdf
collection DOAJ
language English
format Article
sources DOAJ
author N. Singh
N. Singh
C. Deverapalli
G. Khazanov
spellingShingle N. Singh
N. Singh
C. Deverapalli
G. Khazanov
Electrodynamics in a very thin current sheet leading to magnetic reconnection
Nonlinear Processes in Geophysics
author_facet N. Singh
N. Singh
C. Deverapalli
G. Khazanov
author_sort N. Singh
title Electrodynamics in a very thin current sheet leading to magnetic reconnection
title_short Electrodynamics in a very thin current sheet leading to magnetic reconnection
title_full Electrodynamics in a very thin current sheet leading to magnetic reconnection
title_fullStr Electrodynamics in a very thin current sheet leading to magnetic reconnection
title_full_unstemmed Electrodynamics in a very thin current sheet leading to magnetic reconnection
title_sort electrodynamics in a very thin current sheet leading to magnetic reconnection
publisher Copernicus Publications
series Nonlinear Processes in Geophysics
issn 1023-5809
1607-7946
publishDate 2006-01-01
description We study the formation of a very thin current sheet (CS) and associated plasma electrodynamics using three-dimensional (3-D) particle-in-cell simulations with ion to electron mass ratio M/m=1836. The CS is driven by imposed anti-parallel magnetic fields. The noteworthy features of the temporal evolution of the CS are the following: (i) Steepening of the magnetic field profile B<sub>x</sub>(z) in the central part of the CS, (ii) Generation of three-peak current distribution with the largest peak in the CS center as B<sub>x</sub>(z) steepens, (iii) Generation of converging electric fields forming a potential well in the CS center in which ions are accelerated. (iv) Electron and ion heating in the central part of the CS by current-driven instabilities (CDI). (v) Re-broadening of the CS due to increased kinetic plasma pressure in the CS center. (vi) Generation of electron temperature anisotropy with temperature perpendicular to the magnetic field being larger than the parallel one. (vii) Current disruption by electron trapping in an explosively growing electrostatic instability (EGEI) and electron tearing instability (ETI). (viii)The onset of EGEI coincides with an increase in the electron temperature above the temperature of the initially hot ions as well as the appearance of new shear in the electron drift velocity. (ix) Bifurcation of the central CS by the current disruption. (x) Magnetic reconnection (MR) beginning near the null in B<sub>x</sub> and spreading outward. (xi) Generation of highly energized electrons reaching relativistic speeds and having isotropic pitch-angle distribution in the region of reconnected magnetic fields. We compare some of these features of the current sheet with results from laboratory and space experiments.
url http://www.nonlin-processes-geophys.net/13/509/2006/npg-13-509-2006.pdf
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