The classification of Ni XI to XVII and Co X to XVII emission lines from 3s<sup>2</sup> 3p<sup>n</sup>-3s 3p<sup>n+1</sup> and 3p<sup>n</sup>-3p<sup>n-1</sup> 3d transitions and the identification of nickel solar lines
B C Fawcett; R W Hayes; B C Fawcett; Sci. Res. Council., Abingdon, UK; R W Hayes; Sci. Res. Council., Abingdon, UK
Журнал:
Journal of Physics B: Atomic and Molecular Physics
Дата:
1972-02-01
Аннотация:
The 3s<sup>2</sup> 3p<sup>n</sup>-3s 3p<sup>n+1</sup> and 3p<sup>n</sup>-3p<sup>n-1</sup> 3d transitions in Ni XI to XVII and Co X to XVII are classified as a result of the analysis of the spectra emitted from a theta-pinch plasma containing small percentages of nickel or cobalt carbonyl. The nickel lines account for a number of lines in the solar spectrum between 140 AA and 300 AA. The observations check the identity of six coronal forbidden lines.
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