A study of the magnetically sensitive line Fe I 5324.191

Details A study of the magnetically sensitive line Fe I 5324.191 A study of the magnetically sensitive line Fe I 5324.191

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acaps...3..183j&link_type=abstract

(Acta Astrophysica Sinica, vol. 3, no. 3, 1983, p. 183-188) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7, Dec. 19

Astronomy and Astrophysics

Astrophysics

2

Line Spectra, Magnetic Field Configurations, Magnetic Signatures, Solar Magnetic Field, Magnetic Spectroscopy, Stellar Models, Sunspots, Temperature Dependence

Scientific paper

The profiles of the Stokes parameters for the spectral line Fe I wavelength 5324.191 are obtained by numerically solving the Unno equations. The line is found to have a large magnetic intensification and to be not excessively temperature-sensitive. It is concluded that the line is suitable for use as the working line of video-magnetic graphs.

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