Plasmoid instability in the semi-collisional regime
Pallavi Bhat, Nuno Loureiro

TL;DR
This paper analytically and numerically studies the semi-collisional plasmoid instability regime, predicting its existence at lower Lundquist numbers and validating it through gyrokinetic simulations, with implications for experimental observation.
Contribution
It introduces and validates the semi-collisional regime of plasmoid instability, showing it occurs at lower Lundquist numbers than previously thought, using reduced gyrokinetic simulations.
Findings
Plasmoid instability occurs at Lundquist numbers as low as ~250.
The semi-collisional regime exists within specific bounds of S related to L and ρ_S.
Self-consistent formation of current sheets during nonlinear evolution was demonstrated.
Abstract
We investigate analytically and numerically the semi-collisional regime of the plasmoid instability, defined by the inequality , where is the width of a Sweet-Parker current sheet, is the ion sound Larmor radius, and is width of boundary layer that arises in the plasmoid instability analysis. Theoretically, this regime is predicted to exist if the Lundquist number and the length of the current sheet are such that (for a sinusoidal-like magnetic configuration; for a Harris-type sheet the lower bound is replaced with ). These bounds are validated numerically by means of simulations using a reduced gyrokinetic model (Zocco & Schekochihin, , , 2011) conducted with the code . Importantly, this regime is…
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Taxonomy
TopicsDust and Plasma Wave Phenomena · Solar and Space Plasma Dynamics · Fluid Dynamics and Turbulent Flows
