The static equilibrium of axial-symmetric magnetic flux tube

Details The static equilibrium of axial-symmetric magnetic flux tube The static equilibrium of axial-symmetric magnetic flux tube

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981scisn..24.1680h&link_type=abstract

Scientia Sinica, vol. 24, Dec. 1981, p. 1680-1693.

Physics

4

Magnetic Field Configurations, Magnetic Flux, Solar Atmosphere, Solar Flares, Solar Magnetic Field, Thermodynamic Equilibrium, Boundary Value Problems, Chromosphere, Magnetohydrodynamics, Photosphere, Pressure Distribution, Spherical Coordinates, Temperature Distribution

Scientific paper

Features of the solar magnetic flux tube are discussed. Series solutions of the exact nonlinear equations are obtained by expanding the polar angle in the spheric coordinate system for the boundary value problem of the static equilibrium configuration. Results indicate that the magnetic field will be strengthened in the flux tube when the transversal temperature has nonuniform distribution. The magnetic flux tube tends to contract at the lower photosphere and expand at both sides, and the magnetic force lines are twisted in the magnetic surface. An expanding solution is applied in the discussion of the features of the magnetic field configurations, and typical models of the flux tube are described.

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