Oscillator strengths from the solar spectrum

Details Oscillator strengths from the solar spectrum Oscillator strengths from the solar spectrum

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...77..137t&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 77, no. 1, Jan. 1989, p. 137-154.

Astronomy and Astrophysics

Astrophysics

174

Oscillator Strengths, Solar Atmosphere, Solar Spectra, Absorption Spectra, Abundance, Atomic Spectra, Chemical Elements, Photosphere

Scientific paper

Delbouille's (1973) solar spectrum data for the 4006-5684-A region are used to obtain oscillator strengths for 4597 lines identified by Moore et al. (1966). These lines are shown to correspond to 35 chemical elements. The present data are compared with the precise measurements of Blackwell et al. (1983). A precision for log gf of + or - 0.05 dex is found for the unblended lines.

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