Changes of the Fe I spectral line parameters as a function of the magnetic field (solar disk center)

Details Changes of the Fe I spectral line parameters as a function of the magnetic field (solar disk center) Changes of the Fe I spectral line parameters as a function of the magnetic field (solar disk center)

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kfnt....9....8b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 9, no. 3, p. 8-22.

Astronomy and Astrophysics

Astronomy

4

Magnetic Flux, Metallicity, Solar Granulation, Solar Magnetic Field, Spectral Line Width, Fourier Transformation, Iron, Solar Convection (Astronomy)

Scientific paper

The parameter variations of 281 Fe I lines (asymmetry, depth, equivalent width, and halfwidth) are analyzed in three regions near the solar disk center having different magnetic fluxes. The analysis shows that the line parameter variations depend on the line strength, the lower excitation potential, and the line sensitivity to the magnetic field. A qualitative interpretation of the results is given.

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