Determination of iron abundance in the solar atmosphere according to faint-line profiles of ion absorption

Details Determination of iron abundance in the solar atmosphere according to faint-line profiles of ion absorption Determination of iron abundance in the solar atmosphere according to faint-line profiles of ion absorption

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...61b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Jan.-Feb. 1985, p. 61-65. In Russian.

Physics

Absorption Spectra, Abundance, Fraunhofer Lines, Iron, Solar Atmosphere, Spectral Energy Distribution, Atmospheric Models, Ion Motion, Line Shape, Oscillator Strengths, Velocity Distribution

Scientific paper

The iron abundance in the solar atmosphere is obtained as 7.56 + or - 0.06 in the Blackwell oscillator strength system on the basis of 27 Fe II absorption line profiles and Vernazza et al., HSRA, and Holweger-Mueller model atmospheres. The influence of model atmosphere, damping constant, velocity field, and oscillator strength system on the derived abundance is examined.

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