Note on the interpretation of Fe I lines /2.18-2.49 eV/ in the solar spectrum

Details Note on the interpretation of Fe I lines /2.18-2.49 eV/ in the solar spectrum Note on the interpretation of Fe I lines /2.18-2.49 eV/ in the solar spectrum

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199...33b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 199, Apr. 1982, p. 33-36.

Astronomy and Astrophysics

Astronomy

56

Abundance, Iron, Solar Spectra, Spectral Line Width, Electron Oscillations, Line Spectra, Solar Atmosphere, Spectrum Analysis

Scientific paper

Fourteen Fe I lines (2.18 eV < χ < 2.4eV) in the centre of disc solar spectrum are analysed using Oxford oscillator strengths of 1 per cent accuracy. The iron abundances and microturbulence velocities given by these lines are discussed. The five lines with excitation energies 2.40-2.48 eV apparently give a higher abundance than the nine lines of excitation energy 2.18-2.22eV.

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