Sunspot models with twisted magnetic field

Details Sunspot models with twisted magnetic field Sunspot models with twisted magnetic field

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...88..109o&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 88, Oct. 1983, p. 109-115.

Physics

9

Astronomical Models, Magnetic Field Configurations, Solar Magnetic Field, Sunspots, Magnetohydrodynamics, Mathematical Models, Solar Physics

Scientific paper

The return-flux sunspot model is generalized by including azimuthal magnetic field Bφ. The basic equation is obtained and numerical solutions are compared with the analogous solutions for the Schlüter-Temesvary sunspot theory for two cases: Bφ ≡ Br and Bφ ≡ rBr. The solutions demonstrate that the twisting of the sunspot magnetic field decreases with height. The authors' models confirm Yun's early statement: the azimuthal field only slightly influences sunspot structure.

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