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Strongly localized magnetic reconnection by the super-Alfvenic shear flow

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arxiv 1806.00533 v1 pith:WZ3Z4QGL submitted 2018-06-01 physics.plasm-ph astro-ph.EPastro-ph.HEphysics.space-ph

classification physics.plasm-phastro-ph.EPastro-ph.HEphysics.space-ph
keywords reconnectionmagneticratex-lineexplainedfieldordershear
verification ladder T0 review T1 audit T2 compute T3 formal
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We demonstrate the dragging of the magnetic field by the super-Alfvenic shear flows out of the reconnection plane can strongly localize the reconnection x-line in collisionless plasmas, reversing the current direction at the x-line. Reconnection with this new morphology, which is impossible in resistive-magnetohydrodynamic (MHD), is enabled by electron inertia. Surprisingly, the quasi-steady reconnection rate remains of order 0.1 even though the aspect ratio of the local x-line geometry is larger than unity. We explain this by examining the transport of the reconnected magnetic flux and the opening angle made by the upstream magnetic field, concluding that the reconnection rate is still limited by the constraint imposed at the inflow region. This study further suggests the nearly universal fast rate value of order 0.1 cannot be explained by the physics of tearing modes, nor can it be explained by a universal localization mechanism.

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