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Kelvin-Helmholtz instabilities of supersonic/super-alfvenic shear layers

Thesis/Dissertation ·
OSTI ID:6739677
A number of space and astrophysical plasma configurations are characterized by velocity shear layers with a velocity change ..delta..v/sub z/ across a layer of thickness ..delta..x. This thesis examines the stability properties of finite-thickness compressible shear layers. Two different velocity profiles are investigated in detail using the analogy between the pressure perturbation and the bound and scattering wave states of the one-dimensional Schroedinger equation. By analytical and numerical methods, fairly complete contour maps were generated for the real and imaginary parts of the wave frequency as a function of the two free dimensionless parameters, the reduced Mach number, and the wavenumber. Two distinct regimes of instability are delineated. In one regime there are unstable standing waves which are analogous to the well-known Kelvin-Helmholtz warning instability of a vortex sheet (where v/sub z/(x) is a step function). In the second regime, there are unstable travelling wave modes that are absent in the case of a vortex sheet. The stability of finite-thickness, compressible, magnetized shear layers is also investigated numerically. Both the standing and travelling waves are found to occur. A formation is derived for investigating the stability of low temperature, collisionless shear layers in the presence of a magnetic field parallel to the macroscopic flow. The equations of kinetic theory are employed.
Research Organization:
Cornell Univ., Ithaca, NY (USA)
OSTI ID:
6739677
Country of Publication:
United States
Language:
English