The Faraday rotation of sunspots

Details The Faraday rotation of sunspots The Faraday rotation of sunspots

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..112..305y&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 112, no. 2, 1987, p. 305-312.

Physics

2

Faraday Effect, Iron, Line Spectra, Solar Magnetic Field, Sunspots, Error Analysis, Linear Polarization

Scientific paper

The numerical solutions of the Unno-Beckers equations for the magneto-sensitive line Fe I λ5250.216 are used to demonstrate the importance and role of Faraday rotation in sunspot magnetic fields and to study the influence of this effect on the measurements of the azimuth of the transverse field. The authors propose a method to determine the intrinsic direction of the transverse field with the observed azimuthal angle of the plane of linear polarization.

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