An observational examination of models for sunspot magnetic field configurations

Details An observational examination of models for sunspot magnetic field configurations An observational examination of models for sunspot magnetic field configurations

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..125...37a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 125, Jan. 1990, p. 37-44.

Physics

24

Solar Magnetic Field, Stellar Models, Sunspots, Magnetic Field Configurations, Plasma Interactions

Scientific paper

The magnetic field configuration for an isolated, nearly circular sunspot has been obtained from measurements at some 100 points in the spot. The observations are compared with theoretical models for the field configuration of an isolated, axially-symmetric sunspot. The results support the Schlueter, Temesvary model with no return flux and a limiting field line inclination of about 70 deg.

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