Equilibrium and stability of magnetic flux ropes on the sun

Details Equilibrium and stability of magnetic flux ropes on the sun Equilibrium and stability of magnetic flux ropes on the sun

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..465s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Sept. 1979, p. 465-469.) Soviet Astronomy Letters, vol. 5, Sept.-Oct. 1979, p. 250-2

Astronomy and Astrophysics

Astronomy

3

Magnetic Flux, Plasma Equilibrium, Solar Magnetic Field, Solar Wind, Equilibrium Equations, Magnetohydrodynamic Stability, Plasma Cylinders, Solar Atmosphere

Scientific paper

The equilibrium and stability of shielded magnetic flux ropes in the plasma of the solar atmosphere are considered for the case of ropes expanding uniformly along their minor radius. As the rope rises to the surface, such an expansion could result in violation of both the necessary and the sufficient conditions for stability against spiral modes, thereby producing fine structure in the rope magnetic field. However, external disruptive forces would be needed to split the rope into separate strands.

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