A new magneto-hydrostatic theory of sunspots

Details A new magneto-hydrostatic theory of sunspots A new magneto-hydrostatic theory of sunspots

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77...63o&link_type=abstract

Solar Physics, vol. 77, Apr. 1982, p. 63-68.

Computer Science

Numerical Analysis

54

Magnetic Field Configurations, Magnetohydrostatics, Photosphere, Solar Magnetic Field, Sunspots, Astronomical Models, Magnetic Flux, Numerical Analysis

Scientific paper

The structure of a stationary sunspot of circular shape is considered. Schluter-Temesvary theory, based on the 'similarity assumption' is criticized. It is shown that this theory does not describe the observed inclination of magnetic field lines in a sunspot. A new assumption is proposed taking into account field lines which return to the photosphere. On the basis of this assumption, the main equation of the new theory is obtained and the results compare well with observations.

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