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Three‐dimensional collisionless magnetic reconnection in the presence of a guide field

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TLDR
In this article, the authors used 3D particle-in-cell simulations with an open geometry to investigate the changes in the reconnection physics produced by a "guide field" component B0y of the magnetic field.
Abstract
[1] Previous investigations of collisionless magnetic reconnection in a standard Harris neutral sheet configuration have demonstrated the importance of the Hall term for producing near-Alfvenic rates of reconnection and the existence of a very thin (∼c/ωpe) electron current layer and sharp density/pressure gradients on c/ωpi scales. The present work uses three-dimensional (3-D) particle-in-cell simulations with an open geometry to investigate the changes in the reconnection physics produced by a “guide field” component B0y of the magnetic field. With B0y ≲ B0, the nonlinear reconnection rate is not substantially modified from that for the Harris case. The properties of the reconnection fields and particle dynamics, however, are strongly altered. The familiar quadrupole By pattern is replaced by an enhancement of ∣By∣ between the separatrices. The enhanced parallel electric field and parallel electron velocity are confined to one pair of separatrix arms (which are positively charged), while the electron current peaks on the other pair (which are negatively charged). The ion outflow along the current sheet polarizes the separatrices, thereby creating large components of the in-plane electric field. The electrons are accelerated to form a beam structure with parallel speed limited by the electron Alfven speed. The beam-dominated electron distribution produces some y-dependent structures in E∥. For B0y ≫ B0, the reconnection rate is reduced by a factor of 2–3, and the parallel fields and velocities are somewhat smaller; the Hall current produced perturbations in By are considerably reduced.

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Citations
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Electron acceleration from contracting magnetic islands during reconnection

TL;DR: Here it is shown that electrons gain kinetic energy by reflecting from the ends of the contracting ‘magnetic islands’ that form as reconnection proceeds, analogous to the increase of energy of a ball reflecting between two converging walls.
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Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations

TL;DR: Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations were presented in this article, where the authors compared simulations and simulations of the two models.
Journal ArticleDOI

Dipolarization fronts as a signature of transient reconnection in the magnetotail

TL;DR: In this paper, it is shown that bipolarization fronts (DFs) form when the force balance is already restored in the system and justify their interpretation as a nonlinear stage of the tearing instability developing in two magnetotail-like structures on the left and on the right of the initial central X-line.
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Formation of secondary islands during magnetic reconnection

TL;DR: In this paper, full particle simulations are presented that suggest that the strength of an ambient guide magnetic field can determine whether magnetic reconnection remains steady or becomes bursty during anti-parallel (component) reconnection.
References
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Journal ArticleDOI

Numerical solution of initial boundary value problems involving maxwell's equations in isotropic media

Abstract: Maxwell's equations are replaced by a set of finite difference equations. It is shown that if one chooses the field points appropriately, the set of finite difference equations is applicable for a boundary condition involving perfectly conducting surfaces. An example is given of the scattering of an electromagnetic pulse by a perfectly conducting cylinder.
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Theoretical models of magnetic field line merging

TL;DR: A review of the models of magnetic field line merging is given in this paper, where the authors describe the process whereby plasma flows across a surface which separates regions including topologically different magnetic field lines.
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Geospace Environmental Modeling (GEM) magnetic reconnection challenge

TL;DR: In this paper, a simple Harris sheet configuration with a specified set of initial conditions, including a finite amplitude, magnetic island perturbation to trigger the dynamics of magnetic reconnection is studied.
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On a plasma sheath separating regions of oppositely directed magnetic field

TL;DR: In this article, an exact solution of the Vlasov equations was found which describes a layer of plasma confined between two regions of oppositely directed magnetic field, and the electrons and ions have Maxwellian distributions on the plane where the magnetic field vanishes.
Journal ArticleDOI

Dissipation of Currents in Ionized Media

TL;DR: In this article, the fastest stable drift was calculated (drift energy $0.9kT$) and the energy of a faster drift was found to be dissipated into instabilities within, typically, 30 plasma periods.
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