Linear theory of the Kelvin-Helmholtz instability in the low-latitude boundary layer

Details Linear theory of the Kelvin-Helmholtz instability in the low-latitude boundary layer Linear theory of the Kelvin-Helmholtz instability in the low-latitude boundary layer

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jgr....96.9615r&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 96, June 1, 1991, p. 9615-9625. NASA-supported research.

Physics

10

Atmospheric Boundary Layer, Earth Magnetosphere, Kelvin-Helmholtz Instability, Magnetosheath, Plasma Layers, Magnetic Flux, Magnetohydrodynamics, Shear Layers, Tropical Regions

Scientific paper

The feasibility is examined of establishing characteristic profiles across the magnetospheric low-latitude boundary layer for the Kelvin-Helmholtz mode so that these profiles can be compared with satellite observations or a latitudinal chain of ground stations. An anisotropic collisionless fluid model is used instead of conventional MHD, and the finite thickness of the boundary layer and the thickness and position of the current layer are taken into account. The instability is found to be enhanced by a decrease in the thickness of the shear layer and of the current layer and by the proximity of the 'current layer' to the outer edge of the shear layer. The velocity threshold for the onset of instability is insensitive to the thickness. Characteristic profiles of the variation of plasma and field parameters across the boundary are obtained, and the importance of parameters specifying the current layer position and thickness is demonstrated.

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