Nonlinear Acceleration Mechanism of Collisionless Magnetic Reconnection
M. Hirota, P. J. Morrison, Y. Ishii, M. Yagi, N. Aiba

TL;DR
This paper presents an analytical study of a nonlinear acceleration mechanism in collisionless magnetic reconnection, explaining rapid energy release in plasma phenomena like sawtooth crashes in tokamaks.
Contribution
It introduces an analytical estimate of nonlinear tearing mode growth driven by electron inertia, revealing how potential energy decreases steeply and accelerates reconnection.
Findings
Nonlinear potential energy decrease is steeper than linear regime.
Reconnection acceleration is driven by electron inertia effects.
The results support the inertia-driven collapse model of sawtooth crashes.
Abstract
A mechanism for fast magnetic reconnection in collisionless plasma is studied for understanding sawtooth collapse in tokamak discharges. Nonlinear growth of the tearing mode driven by electron inertia is analytically estimated by invoking the energy principle for the first time. Decrease of potential energy in the nonlinear regime (where the island width exceeds the electron skin depth) is found to be steeper than in the linear regime, resulting in acceleration of the reconnection. Release of free energy by such ideal fluid motion leads to unsteady and strong convective flow, which theoretically corroborates the inertia-driven collapse model of the sawtooth crash [D. Biskamp and J. F. Drake, Phys. Rev. Lett. 73, 971 (1994)].
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Taxonomy
TopicsMagnetic confinement fusion research · Solar and Space Plasma Dynamics · Magnetic Field Sensors Techniques
