Physics
Scientific paper
Oct 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...38..343a&link_type=abstract
Solar Physics, vol. 38, Oct. 1974, p. 343-350.
Physics
29
Photosphere, Radiative Lifetime, Radioactive Decay, Rare Earth Elements, Solar Atmosphere, Abundance, Cerium, Line Spectra, Lutetium, Praseodymium, Thallium, Transition Probabilities
Scientific paper
Radiative lifetimes have been determined by the beam-foil method for some excited states in the singly ionized rare earths Pr II, Tm II, and Lu II, in order to test the reliability of the transition probabilities and oscillator strengths found by Corliss and Bozman and usually applied for solar abundance determinations. Correction factors of 4.5, 2.5, and 0.3 should be applied to Corliss and Bozman's values for Pr II, Tm II, and Lu II, respectively. These corrections eliminate the discrepancies between the abundance in the solar photosphere and in meteorites for Pr and Tm. Radiative lifetimes for Ce III are also reported.
Andersen Torsten
Sorensen G.
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