Physics
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...61...17b&link_type=abstract
Solar Physics, vol. 61, Feb. 1979, p. 17-22. Research supported by the Fonds de la Recherche Fondamentale Collective.
Physics
15
Abundance, Photosphere, Praseodymium, Solar Spectra, Hyperfine Structure, Spectrum Analysis
Scientific paper
Sixteen lines of Pr II possibly present in the solar photospheric
spectrum have been studied. When hyperfine structure is included in
synthetic calculations, investigations of nine lines result in a
logarithmic Pr abundance of 0.71 plus or minus 0.08 on the scale where
the logarithmic H abundance is 12.00.
Biémont É.
Grevesse Nicolas
Hauge O.
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