Mathematics
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21.1044m&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 21, Nov.-Dec. 1981, p. 1044-1047. In Russian.
Mathematics
1
Boundary Layers, Equatorial Atmosphere, Kelvin-Helmholtz Instability, Magnetospheric Instability, Algorithms, Atmospheric Models, Flow Velocity, Plasma Density
Scientific paper
A theoretical analysis is presented of the effect of the structure of plasma density and velocity distributions in the low-latitude magnetospheric boundary layer on the excitation conditions of the Kelvin-Helmholtz instability. The mathematical model and the algorithm used in the analysis are described in detail, and numerical results are presented. It is shown that, in the case of a sufficiently large plasma-density drop, the boundary of the instability is displaced toward the short-wave region.
Mishin V. V.
Morozov A. G.
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