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The Vlasov model under large magnetic fields in the low-Mach number regime

2009/05/14 by Pierre Degond, Degond, Pierre, Sever A. Hirstoaga +3
Physics and Astronomy · #FOS: Physical sciences #Ionosphere and magnetosphere dynamics #Laser-Plasma Interactions and Diagnostics #Magnetic confinement fusion research #Mathematical Physics (math-ph)

paper · pdf · doi:10.48550/arxiv.0905.2400

openalex publication_date 2009/05/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

This article is concerned with the kinetic modeling, by means of the Vlasov equation, of charged particles under the influence of a strong external electromagnetic field, i.e. when epsilon2, the dimensionless cyclotron period, tends to zero. This leads us to split the velocity variable in the Vlasov equation into fluid and random components. The latter is supposed to have a large magnitude of order 1/epsilon (which corresponds to the low Mach number regime). In the limit epsilon -> 0, the resulting model is a hybrid model which couples a kinetic description of the microscopic random motion of the particles to a fluid description of the macroscopic behavior of the plasma. The microscopic model is a first-order partial differential system for the distribution function, which is averaged over the ultra-fast Larmor gyration and the fast parallel motion along the magnetic field lines. The perpendicular component (with respect to the magnetic field lines) of the bulk velocity is governed by the classical relations describing the E X B and diamagnetic drifts, while its parallel component satisfies an elliptic equation along the magnetic field lines.

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