The spiral configuration of sunspot magnetic fields

Physics

Scientific paper

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Magnetic Field Configurations, Polarization Characteristics, Solar Magnetic Field, Sunspots, Astronomical Models, Magnetic Flux, Magnetometers, Solar Spectra

Scientific paper

Distributions of circularly and linearly polarized intensities are computed using an analytical magnetic field model for an isolated sunspot, and these intensity distributions are compared with observed intensities in all Stokes parameters in the 5250-A line measured with the Marshall Space Flight Center's vector magnetograph. The qualitative agreement between measured and calculated linearly polarized intensity distributions is discussed with regard to implications as to the configuration of the transverse magnetic field of the isolated sunspot.

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