Energy levels and oscillator strengths are calculated for the 3s23pn-3s23pn-13dtransition arrays of Fe X and Fe XI. The Slater radial integrals for these computations are adjusted so as to become consistent with established energy levels. Pertinent configuration interactions are included and the interaction integrals are reduced by up to 35% from values calculatedab initio, to achieve consistency. Predictions from this analysis lead to new line identifications in solar and laboratory spectra.
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Bromage et al. (1977) studied this question.
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