Velocity boundary layers in the distant geotail and the Kelvin Helmholtz instability

Details Velocity boundary layers in the distant geotail and the Kelvin Helmholtz instability Velocity boundary layers in the distant geotail and the Kelvin Helmholtz instability

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005p%26ss...53..157m&link_type=abstract

Planetary and Space Science, Volume 53, Issue 1-3, p. 157-160.

Physics

1

Scientific paper

The formation of velocity boundary layers at the flanks of the distant
geotail due to the Kelvin Helmholtz instability has been studied. It is
shown that the build-up of slow oblique perturbations leads to an
anomalous viscosity sufficient for the formation of thick boundary
layers in the distant magnetotail.

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