Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988sssmp..31..192h&link_type=abstract
Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 31, Feb. 1988, p.
Astronomy and Astrophysics
Astronomy
Magnetic Field Configurations, Magnetostatics, Penumbras, Perturbation Theory, Solar Magnetic Field, Sunspots, Cylindrical Coordinates, Hyperbolic Differential Equations, Partial Differential Equations, Photosphere
Scientific paper
The perturbation theory is applied further to the discussion of the equilibrium properties of a sunspot-like magnetic field with a strong twisted component. The basic state reduces to the usual one discussed extensively for the axisymmetric magnetostatic equilibrium with a twisted component of the magnetic field, and the perturbed state is described by two coupled equations. As the magnetic force-line is twisted, there is a magnetic tension in the azimuthal direction. In this case, the perturbed total pressure is no longer independent of the azimuthal variable and the magnetic field in the dark penumbal fibril may be either stronger or weaker relatively.
Hu Wenrui
Long Hui
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