Numerical Studies of Weakly Stochastic Magnetic Reconnection
G. Kowal, A. Lazarian, E. T. Vishniac, K. Otmianowska-Mazur

TL;DR
This study uses 3D numerical simulations to test a model of fast magnetic reconnection influenced by turbulence, confirming the model's predictions and elucidating how turbulence parameters affect reconnection rates.
Contribution
First numerical validation of the Lazarian & Vishniac (1999) model showing turbulence enhances reconnection speed and alters magnetic topology.
Findings
Reconnection speed scales as V^2 with turbulence velocity amplitude.
Reconnection rate depends on injection scale as (l/L)^(2/3).
Global reconnection rate is independent of resistivity in turbulent conditions.
Abstract
We study the effects of turbulence on magnetic reconnection using three-dimensional numerical simulations. This is the first attempt to test a model of fast magnetic reconnection proposed by Lazarian & Vishniac (1999), which assumes the presence of weak, small-scale magnetic field structure near the current sheet. This affects the rate of reconnection by reducing the transverse scale for reconnection flows and by allowing many independent flux reconnection events to occur simultaneously. We performed a number of simulations to test the dependencies of the reconnection speed, defined as the ratio of the inflow velocity to the Alfven speed, on the turbulence power, the injection scale and resistivity. Our results show that turbulence significantly affects the topology of magnetic field near the diffusion region and increases the thickness of the outflow region. We confirm the predictions…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
