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arxiv: 1711.06708 · v1 · pith:5NEKDSYGnew · submitted 2017-11-17 · ⚛️ physics.plasm-ph · astro-ph.SR· physics.space-ph

On the collisionless asymmetric magnetic reconnection rate

classification ⚛️ physics.plasm-ph astro-ph.SRphysics.space-ph
keywords reconnectionrateasymmetricfieldmagneticmodelcollisionlessfactor
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A prediction of the steady-state reconnection electric field in asymmetric reconnection is obtained by maximizing the reconnection rate as a function of the opening angle made by the upstream magnetic field on the weak magnetic field (magnetosheath) side. The prediction is within a factor of two of the widely examined asymmetric reconnection model [Cassak and Shay, Phys. Plasmas 14, 102114, 2007] in the collisionless limit, and they scale the same over a wide parameter regime. The previous model had the effective aspect ratio of the diffusion region as a free parameter, which simulations and observations suggest is on the order of 0.1, but the present model has no free parameters. In conjunction with the symmetric case [Liu et al., Phys. Rev. Lett. 118, 085101, 2017], this work further suggests that this nearly universal number 0.1, essentially the normalized fast reconnection rate, is a geometrical factor arising from maximizing the reconnection rate within magnetohydrodynamic (MHD)-scale constraints.

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