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A magnetostatic sunspot model with ‘twisted’ field

✍ Scribed by Hong Sik Yun

Publisher
Springer
Year
1971
Tongue
English
Weight
276 KB
Volume
16
Category
Article
ISSN
0038-0938

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✦ Synopsis

It is shown that the internal structure of sunspots is affected only to a small degree by the presence of the azimuthal component of the sunspot magnetic field. The magnetostatic theory of sunspots developed by Schltiter and Temesvary (1958) is extended to include such an effect. In the present study, the radial dependence of the azimuthal component of the field is adopted from the observation of Stepanov (1965). A typical sunspot of an effective temperature of 4000 K is considered and its detailed structure is presented. * Publications of the Goethe Link Observatory, No. 115.

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