Magnetic reconnection and plasmoid formation driven by the two-dimensional resistive kink instability in a current hole configuration
Hubert Baty

TL;DR
This study explores how the resistive internal kink mode in a 2D current hole configuration leads to magnetic reconnection and plasmoid formation, revealing a transition from Sweet-Parker to plasmoid-dominated regimes at high Lundquist numbers.
Contribution
It demonstrates the nonlinear evolution of the resistive kink mode and identifies the critical Lundquist number for plasmoid formation in a current hole setup.
Findings
Reconnection rate of approximately 0.02 observed.
Plasmoid formation occurs when Lundquist number exceeds ~10^4.
Transition from Sweet-Parker to plasmoid-dominated reconnection regimes.
Abstract
We investigate the nonlinear evolution of the resistive internal kink mode in a two-dimensional (2D) configuration containing a central region of negative current density, also known as the "current hole" setup. The finite-element code FINMHD is used to solve a reduced set of incompressible Magnetohydrodynamic (MHD) equations with a current-vorticity formulation. First, the kink instability linearly develops in agreement with the general theory of resistive internal kink mode, and it subsequently leads to the formation of a current sheet. At relatively low Lundquist number , a magnetic reconnection process proceeds with a rate predicted by the Sweet-Parker regime. Conversely, when exceeds a critical value that is , the current sheet is disrupted by the formation of plasmoids on a slightly sub-Alfv\'enic time scale. In the latter case, a stochastic…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Fluid Dynamics and Turbulent Flows · Magnetic confinement fusion research
