pith. sign in

arxiv: 0704.2758 · v1 · pith:FER2EZYLnew · submitted 2007-04-20 · ⚛️ physics.space-ph · astro-ph

The Orientation of the Reconnection X-line

classification ⚛️ physics.space-ph astro-ph
keywords x-linereconnectionfieldsmagneticorientationalfvangleapproximation
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.