Oscillator strengths and damping constants from the solar spectrum at 830-870 NM

Details Oscillator strengths and damping constants from the solar spectrum at 830-870 NM Oscillator strengths and damping constants from the solar spectrum at 830-870 NM

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...80..229e&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 80, no. 2, Oct. 1989, p. 229-237. Research supported by FAPE

Astronomy and Astrophysics

Astrophysics

13

Atomic Energy Levels, Infrared Spectra, Oscillator Strengths, Photosphere, Solar Spectra, Line Spectra, Molecular Spectra, Spectral Bands

Scientific paper

Oscillator strengths and damping constants in the spectral region from 830 to 870 nm are obtained from a fit to the solar spectrum. The atomic lines considered are those given in Moore et al. (1966) and Swensson et al. (1974). This spectral region comprehends the lines of the CaII infrared triplet, besides several other atomic lines, and the molecular bands of CN A2Pi-X2Sigma system and TiO A3Phi-X3Delta gamma-system. The results are reported together with a comparison to data from the literature.

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