Magneto-optical effects in sunspots and their vector magnetic field

Details Magneto-optical effects in sunspots and their vector magnetic field Magneto-optical effects in sunspots and their vector magnetic field

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acasn..24..119y&link_type=abstract

(Acta Astronomica Sinica, vol. 24, no. 1-3, 1983, p. 119-127) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7, Dec.

Physics

Optics

1

Magnetic Field Configurations, Magneto-Optics, Solar Magnetic Field, Sunspots, Algebra, Field Strength, Graphs (Charts), Vector Analysis

Scientific paper

The Unno-Beckers equations are numerically solved for the magnetosensitive lines Fe I wavelengths 6302.499 and 5324.191 using an appropriate sunspot model. Beckers' (1969) errors in the coefficients representing the magnetooptical effect are corrected and an improved method for computing algebraic solutions to the Unno-Beckers equations is introduced. The numerical solution is used to set up a simple method of deriving the magnetic field strength, the inclination angle of the field, and the azimuthal angle of the field, from the profiles of the four Stokes parameters.

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