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The Orientation of the Reconnection X-line

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arxiv 0704.2758 v1 pith:FER2EZYL submitted 2007-04-20 physics.space-ph astro-ph

classification physics.space-phastro-ph
keywords x-linereconnectionfieldsmagneticorientationalfvangleapproximation
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We propose a criterion for identifying the orientation of the X-line when two regions of plasma with arbitrary densities, temperatures, and magnetic fields undergo reconnection. The X-line points in the direction that maximizes the (suitably-defined) Alfv\'en speed characterizing the reconnection outflow. For many situations a good approximation is that the X-line bisects the angle formed by the magnetic fields.

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