Computation of oscillator strengths by a semi-empirical method for some elements of the iron-group and their solar photospheric abundance. I - Results for TI I

Details Computation of oscillator strengths by a semi-empirical method for some elements of the iron-group and their solar photospheric abundance. I - Results for TI I Computation of oscillator strengths by a semi-empirical method for some elements of the iron-group and their solar photospheric abundance. I - Results for TI I

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...38...15b&link_type=abstract

Solar Physics, vol. 38, Sept. 1974, p. 15-31. Research supported by the Fonds de la Recherche Fondamentale Collective of Belgium

Physics

16

Abundance, Line Spectra, Molecular Oscillations, Photosphere, Solar Spectra, Titanium, Infrared Spectra, Iron, Solar Atmosphere, Tables (Data), Thomas-Fermi Model, Transition Probabilities

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1974SoPh...38...15B

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