Physica Scripta · 1979 · 65 citations · 16 references
Natural SciencesChemistryPhysicsPhysical ChemistryQuantum ChemistrySpectroscopyAb Initio MethodsElectronic SpectroscopyElectronic Structure DeterminationFine Structure TransitionsLow-spin Configurations
Available measurements of the transitions 2s2-2s2p and 2s2p-2p2 are examined as to their iso-electronic consistency by studying appropriate functions of the transition energies of 2s2 1S0-2s2p1P1, 3P1, 2s2p1P1-2p2 1D2, 1S0 and 2s2p3P2-2p2 3P2, and by deriving semi-empirical screening formulae for the fine-structure intervals of the 3P terms. In this way, accidental experimental errors are smoothed out and missing data are determined by interpolation. The results of the analysis are comprised in a table of recommended level values, extending to Z = 26 or, for 2s2p1P1, 3P1, to Z = 28. A comment on our recent discussion of the Li I-like spectra is appended.
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Spectral lines observed in solar flares between 171 and 630 angstroms
K. P. Dere · The Astrophysical Journal · 1978 · 245 citations · Full text
Natural Sciences, Astronomy, Physics +16
The solar spectrum - Wavelengths and identifications from 160 to 770 angstroms
W. E. Behring, L. Cohen, G. A. Doschek et al. · The Astrophysical Journal · 1976 · 190 citations
Natural Sciences, Astronomy, Physics +15