Skinning process stability of the magnetic field in the solar active regions

Details Skinning process stability of the magnetic field in the solar active regions Skinning process stability of the magnetic field in the solar active regions

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51..293s&link_type=abstract

Solar Physics, vol. 51, Mar. 1977, p. 293-306.

Physics

Plasma Physics

2

Magnetohydrodynamic Stability, Plasma Physics, Solar Activity, Solar Magnetic Field, Electrical Resistivity, Gray Gas, Skin Resistance

Scientific paper

The skinning process stability of the magnetic field in homogeneous plasma is studied. A set of magnetohydrodynamic equations is used. The dependence of electrical conductivity on the plasma parameters and radiation intensity in grey-body approximation are taken into account. The investigation is carried out on the model problems in linear approximation and by means of numerical solution of MHD equations. Threshold of stability and critical gradient of magnetic field in skin-layer are obtained. The model of the phenomenon proposed in the paper indicates on overheating instability of plasma with electric current in large gradient magnetic field zones as a possible trigger mechanism of solar flare origin.

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