Oscillator strengths of Fe II lines derived from the solar spectrum - Choice of solar model atmosphere

Details Oscillator strengths of Fe II lines derived from the solar spectrum - Choice of solar model atmosphere Oscillator strengths of Fe II lines derived from the solar spectrum - Choice of solar model atmosphere

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81..340b&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 3, Jan. 1980, p. 340-343.

Astronomy and Astrophysics

Astrophysics

87

Atmospheric Models, Atomic Excitations, Iron, Solar Atmosphere, Solar Spectra, Stellar Models, Abundance, Line Spectra

Scientific paper

The Fe II solar spectrum is interpreted using oscillator strengths measured by Baschek et al., and the results used in conjunction with Fe I analyses to make a choice between the solar model atmospheres of Holweger and Müller, and of Vernazza et al. It is suggested that the Holweger and atmosphere describes these two spectra better. Solar oscillator strengths for 42 lines of Fe II are given with a suggested accuracy of ±015 dex and comparisons made with the calculated values of Kurucz and Peytremann, and measured values.

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