Rapid Change of Field Line Connectivity and Reconnection in Stochastic Magnetic Fields
Yi-Min Huang, A. Bhattacharjee, and Allen H. Boozer

TL;DR
This study investigates how stochastic magnetic fields influence magnetic reconnection, revealing that rapid changes in field line connectivity often lead to enhanced diffusion rather than true reconnection, with fast reconnection occurring mainly during instability onset.
Contribution
The paper demonstrates through simulations that stochasticity causes rapid connectivity changes mainly resulting in diffusion, and identifies conditions under which true reconnection occurs during instability.
Findings
Rapid connectivity change correlates with high field line exponentiation.
Overall field line mapping deforms gradually despite local rapid changes.
Fast reconnection occurs during instability onset, not just from stochasticity.
Abstract
Magnetic fields without a direction of continuous symmetry have the generic feature that neighboring field lines exponentiate away from each other and become stochastic, hence the ideal constraint of preserving magnetic field line connectivity becomes exponentially sensitive to small deviations from ideal Ohm's law. The idea of breaking field line connectivity by stochasticity as a mechanism for fast reconnection is tested with numerical simulations based on reduced magnetohydrodynamics equations with a strong guide field line-tied to two perfectly conducting end plates. Starting from an ideally stable force-free equilibrium, the system is allowed to undergo resistive relaxation. Two distinct phases are found in the process of resistive relaxation. During the quasi-static phase, rapid change of field line connectivity and strong induced flow are found in regions of high field line…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Magnetic confinement fusion research · Ionosphere and magnetosphere dynamics
