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Kinetic theory of magnetohydrodynamic Kelvin--Helmholtz instability

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.861620· OSTI ID:7266478
The magnetohydrodynamic Kelvin--Helmholtz instability in a low ..beta.. collisionless plasma with smooth variations in plasma parameters across the boundary is studied. The surface Alfven wave which is excited by the Kelvin--Helmholtz instability is shown to be mode-converted to the kinetic Alfven wave (Alfven wave with finite ion Larmor radius and electron inertia correction). Linear and nonlinear effects of this kinetic Alfven wave on the Kelvin--Helmholtz instability are discussed. Because the resonant mode conversion enhances the wave amplitude, the nonlinear effect is manifested. In particular, the magnetic field pressure of the kinetic Alfven wave exerts acceleration on the plasma at the higher density side toward the lower density side and may cause the Rayleigh--Taylor instability at the boundary layer. (AIP)
Research Organization:
Department of Physics, Nagoya University, Nagoya, Japan
OSTI ID:
7266478
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 19:8; ISSN PFLDA
Country of Publication:
United States
Language:
English