O III line ratios in the sun

Details O III line ratios in the sun O III line ratios in the sun

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...344..522k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 344, Sept. 1, 1989, p. 522-524. Research supported by SERC.

Astronomy and Astrophysics

Astrophysics

9

Line Spectra, Oxygen Spectra, Solar Spectra, Ultraviolet Spectra, Abundance, Electron Energy, Electron Transitions

Scientific paper

The R-matrix code is used to calculated electron impact excitation rates for transitions in O III. The calculated rates are used to determine the theoretical electron sensitive emission-line ratios R(1) and R(2). The ratios are up to a factor of 2 smaller than those of Bhatia et al. (1982). The results are compared with solar observations from Skylab, showing good agreement.

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