The appearance, motion, and disappearance of three-dimensional magnetic null points
Nicholas A. Murphy, Clare E. Parnell, and Andrew L. Haynes

TL;DR
This paper derives exact expressions for the motion of three-dimensional magnetic null points, revealing how asymmetry, resistive effects, and bifurcations influence their dynamics in magnetic reconnection.
Contribution
It provides a comprehensive analytical framework for understanding null point motion, including during bifurcations, incorporating local parameters and global dynamics.
Findings
Null points move along directions where the vector field and its time derivative are antiparallel.
Null point motion results from plasma advection and resistive diffusion.
Bifurcations can cause null-null pairs to have infinite separation velocity along certain directions.
Abstract
While theoretical models and simulations of magnetic reconnection often assume symmetry such that the magnetic null point when present is co-located with a flow stagnation point, the introduction of asymmetry typically leads to non-ideal flows across the null point. To understand this behavior, we present exact expressions for the motion of three-dimensional linear null points. The most general expression shows that linear null points move in the direction along which the vector field and its time derivative are antiparallel. Null point motion in resistive magnetohydrodynamics results from advection by the bulk plasma flow and resistive diffusion of the magnetic field, which allows non-ideal flows across topological boundaries. Null point motion is described intrinsically by parameters evaluated locally; however, global dynamics help set the local conditions at the null point. During a…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
