Stability of the boundary layer of a skinned magnetic flux rope

Details Stability of the boundary layer of a skinned magnetic flux rope Stability of the boundary layer of a skinned magnetic flux rope

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sval....3..170s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 3, July 1977, p. 319-321.) Soviet Astronomy Letters, vol. 3, July-Aug. 1977, p. 170-172

Astronomy and Astrophysics

Astronomy

1

Boundary Layer Stability, Magnetic Disturbances, Magnetic Flux, Solar Magnetic Field, Azimuth, Magnetic Field Configurations, Solar Atmosphere

Scientific paper

The boundary layer of a skinned (i.e., isolated) magnetic flux rope is defined as that region where the intensity of the azimuthal magnetic field decreases more steeply than in accordance with the 1/r law. The MHD stability of such a boundary layer is analyzed using a certain stability criterion for the case of a linear plasma pinch. It is shown that the boundary layer of a skinned magnetic flux rope is always stable with respect to arbitrary small perturbations.

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