Computation of oscillator strengths by a semiempirical method for some elements of the iron group and their solar photospheric abundance. II - Results for SC I

Details Computation of oscillator strengths by a semiempirical method for some elements of the iron group and their solar photospheric abundance. II - Results for SC I Computation of oscillator strengths by a semiempirical method for some elements of the iron group and their solar photospheric abundance. II - Results for SC I

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..305b&link_type=abstract

Solar Physics, vol. 39, Dec. 1974, p. 305-308. Research supported by the Fonds de la Recherche Fondamentalle Collective.

Physics

7

Abundance, Line Spectra, Photosphere, Scandium, Solar Spectra, Thomas-Fermi Model, Electron Transitions, Fine Structure, Molecular Oscillations, Solar Atmosphere, Spectral Line Width, Transition Probabilities

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1974SoPh...39..305B

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