Computer Science
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...75p&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, May-June 1985, p. 75-77. In Russian.
Computer Science
1
Europium, Photosphere, Solar Atmosphere, Solar Spectra, Stellar Composition, Abundance, Fraunhofer Lines, Spectral Line Width, Spectrum Analysis
Scientific paper
The relative abundance of europium in the undisturbed solar photosphere has been determined on the basis of five Eu II line profiles in the spectral region of 600-740 nm. The Eu II line profiles were derived using an equivalent width technique (four lines), the synthetic spectrum method (one line at a wavelength of 617.304 nm). An Eu abundance of 0.71 + or - 0.08 in the scale log H = 12.00 is given. The results of previous studies of Eu abundance in the solar atmosphere are presented.
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