A comparison of theoretical line strengths for the 2s(2)2p(2)-2s(2)2p(3) transitions in NeV with solar data

Details A comparison of theoretical line strengths for the 2s(2)2p(2)-2s(2)2p(3) transitions in NeV with solar data A comparison of theoretical line strengths for the 2s(2)2p(2)-2s(2)2p(3) transitions in NeV with solar data

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..122....1k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 122, no. 1, 1989, p. 1-6. Research supported by SERC.

Astronomy and Astrophysics

Astronomy

5

Electron Transitions, Line Spectra, Neon, Solar Spectra, Skylab Program, Spaceborne Astronomy

Scientific paper

Results are presented for several theoretical line ratios in NeV involving transitions between multiplets in the 2s(2)2p(2) and 2s2p(3) configurations. A comparison of these with solar data from the SO82A and S-O55 instruments on board Skylab reveals generally good agreement between theory and experiment, especially in the case of the high-resolution (SO82A) observations. However, the 2s(2)2p(2) 1D - 2s(2)p(3) 1P (365.6-A) and 2s(2)2p(2)3P - 2s2p(3) 3S(359-A) lines appear to be blended, possibly with transitions in Fe X and Fe XI/Fe XIII, respectively.

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