On statistical significance of the iron abundance anomaly for 2.2 eV Fe I lines.

Details On statistical significance of the iron abundance anomaly for 2.2 eV Fe I lines. On statistical significance of the iron abundance anomaly for 2.2 eV Fe I lines.

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988bsold...5...88b&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1988/5, p. 88 - 94

Physics

1

Solar Spectrum: Iron

Scientific paper

It is shown that the abundance anomaly of neutral iron lines with the
excitation potential 2.2 eV discovered by Blackwell et al. in the solar
spectrum using Oxford oscillator strengths, becomes statistically
insignificant for larger data sets.

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