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

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

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...44..269b&link_type=abstract

Solar Physics, vol. 44, Oct. 1975, p. 269-273. Research supported by the Fonds de la Recherche Fondamentale Collective.

Physics

12

Abundance, Manganese, Molecular Oscillators, Photosphere, Solar Spectra, Electron Transitions, Fine Structure, Tables (Data)

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1975SoPh...44..269B

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