Magneto-sensitive lines in the solar spectrum

Details Magneto-sensitive lines in the solar spectrum Magneto-sensitive lines in the solar spectrum

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978acasn..19..152y&link_type=abstract

Acta Astronomica Sinica, vol. 19, Dec. 1978, p. 152-165. In Chinese, with abstract in English.

Physics

2

Line Spectra, Radiative Transfer, Solar Magnetic Field, Solar Spectra, Zeeman Effect, Atmospheric Models, Sensitivity, Solar Atmosphere, Solar Physics, Sunspots, Temperature Effects

Scientific paper

A numerical solution of the equations of transfer of the Stokes parameters in the presence of magnetic fields is carried out. This yields the profiles of the Stokes parameters for three magneto-sensitive spectral lines (Fe I lines at 6302.499, 6173.341, and 5250.216 A). The magnetic intensification, temperature sensitivity, and various other properties of the lines are investigated. The numerical solution obtained agrees better with observations than the algebraic solution of Unno.

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