Hyperfine structure and the broadening of sunspot spectral lines

Details Hyperfine structure and the broadening of sunspot spectral lines Hyperfine structure and the broadening of sunspot spectral lines

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984josab...1..311g&link_type=abstract

(NASA, NRC, and University of California, Symposium on Atomic Spectroscopy, Berkeley, CA, Sept. 12-16, 1983) Optical Society of

Physics

3

Hyperfine Structure, Line Spectra, Solar Spectra, Spectral Line Width, Sunspots, Manganese, Zeeman Effect

Scientific paper

The combined effects of hyperfine structure and Zeeman splitting have been calculated for the a6D1/2-z6D1/2 line of Mn I at wavelength 4070.28 Å, which is observed as a broad line in sunspot spectra. An effective Z factor is defined to represent the mean position of the strong components of the line for fields above 500 G. This Z factor might provide a method of monitoring sunspot magnetic fields.

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