On the determination of damping constants for Fe I lines in the solar photosphere

Details On the determination of damping constants for Fe I lines in the solar photosphere On the determination of damping constants for Fe I lines in the solar photosphere

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...67....5v&link_type=abstract

Solar Physics, vol. 67, Aug. 1980, p. 5-7.

Physics

Line Spectra, Photosphere, Solar Spectra, Iron, Spectral Line Width, Tables (Data)

Scientific paper

The line broadening calculated with a Smirnov-Roueff potential, yields a
fairly good description of the intensity profile in the wings of 31
solar Fe I lines.

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