Abstract
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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Deridder, G. and Van Rensbergen, W.: 1976, Astron. Astrophys. Suppl. 23, 147.
Edmunds, M.: 1975, Astron. Astrophys. 38, 137.
Gingerich, O., Noyes, R., Kalkofen, W., and Cuny, Y.: 1971, Solar Phys. 18, 347.
Gurtovenko, E. and Kondrashova, N.: 1980, Solar Phys. (in press).
Moore, C.: 1945, ‘A Multiplet Table of Astrophysical Interest’, NBS Technical Note 36.
Unsöld, A.: 1968, Physik der Sternatmosphären, Springer, Berlin.
Van Rensbergen, W., De Doncker, E., and Deridder, G.: 1975, Solar Phys. 40, 303.
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Van Rensbergen, W., Deridder, G. On the determination of damping constants for Fe I lines in the solar photosphere. Sol Phys 67, 5–7 (1980). https://doi.org/10.1007/BF00146676
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DOI: https://doi.org/10.1007/BF00146676