A detection of the Faraday rotation by the solar vector magnetograph

Details A detection of the Faraday rotation by the solar vector magnetograph A detection of the Faraday rotation by the solar vector magnetograph

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..103....1m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 103, Jan. 1986, p. 1-10.

Physics

9

Faraday Effect, Linear Polarization, Magnetic Signatures, Solar Magnetic Field, Solar Spectra, Sunspots, Azimuth, Line Spectra

Scientific paper

The Faraday rotation in the sunspot atmosphere is statistically detected by examining directions of the linear polarization obtained with the vector magnetograph of the Okayama Astrophysical Observatory. It is very effective near the spectral line center and the azimuth of the linear polarization deviates greatly from the magnetic field azimuth. In the case of the iron line, 5250 Å, the magnetic field azimuth will be obtained with an accuracy better than 15°, if observed in the line wing from 27 to 80 mÅ relative to the line center.

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