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Role of electron inertia and reconnection dynamics in a stressed

By J. Graf von der Pahlen and D. Tsiklauri


Aims. In previous simulations of collisionless 2D magnetic reconnection it was consistently found that the term in the generalised Ohm’s law that breaks the frozen-in condition is the divergence of the electron pressure tensor’s non-gyrotropic components. The motivation for this study is to investigate the effect of the variation of the guide-field on the reconnection mechanism in simulations of X-point collapse, and the related changes in reconnection dynamics. Methods. A fully relativistic particle-in-cell (PIC) code was used to model X-point collapse with a guide-field in two and three spatial dimensions. Results. We show that in a 2D X-point collapse with a guide-field close to the strength of the in-plane field, the increased induced shear flows along the diffusion region lead to a new reconnection regime in which electron inertial terms play a dominant role at the X-point. This transition is marked by the emergence of a magnetic island – and hence a second reconnection site – as well as electron flow vortices moving along the current sheet. The reconnection electric field at the X-point is shown to exceed all lower guide-field cases for a brief period, indicating a strong burst in reconnection. By extending the simulation to three spatial dimensions it is shown that the locations of vortices along the current sheet (visualised by their Q-value) vary in the out-of-plane direction, producing tilted vortex tubes. The vortex tubes on opposite sides of the diffusion region are tilted in opposite directions, similarly to bifurcated current sheets in oblique tearing-mode reconnection. The tilt angles of vortex tubes were compared to a theoretical estimation and were found to be a good match. Particle velocity distribution functions for different guide-field runs, for 2.5D and 3D simulations, are analysed and compared

Topics: magnetic reconnection, magnetic fields, plasmas, Sun: flares, Sun: magnetic fields, Sun: coronal mass ejections (CMEs)
Publisher: 'EDP Sciences'
Year: 2016
DOI identifier: 10.1051/0004-6361/201628071
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