Plasma Mixing Driven by the Collisionless Kelvin-Helmholtz Instability: Insights from fully kinetic simulation and density-based diagnostics
Silvia Ferro, Fabio Bacchini, Giuseppe Arr\`o, Francesco Pucci, Pierre Henri

TL;DR
This study uses high-resolution kinetic simulations to analyze plasma mixing driven by the collisionless Kelvin-Helmholtz instability, revealing localized mixing, species dependence, and the role of magnetic reconnection.
Contribution
It provides new insights into the spatial localization, species dependence, and physical mechanisms of plasma mixing in collisionless shear flows using kinetic simulations.
Findings
Mixing is localized mainly at narrow interface regions.
Ions mix more effectively than electrons, which stay tied to magnetic field lines.
Magnetic reconnection correlates with enhanced plasma mixing.
Abstract
Simulations and observations of the low-latitude magnetosphere-magnetosheath boundary layer indicate that the Kelvin-Helmholtz instability (KHI) drives vortex structures that enhance plasma mixing and magnetic reconnection, influencing transport and particle acceleration. We investigate the spatial localization, species dependence, and physical mechanisms of plasma mixing driven by the nonlinear evolution of the KHI. We perform high-resolution two-dimensional Particle-In-Cell simulations using a finite-Larmor-radius shear-flow initial configuration. Plasma mixing is quantified using particle labeling, a complementary density-based mixing tracer, and diagnostics of magnetic reconnection. Mixing across the shear layer is present but localized, occurring mainly in narrow interface regions and plasma structures. Ions mix more effectively than electrons, which remain largely frozen to field…
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