Corrected fine-structure energy levels and oscillator strengths for Ne i–Si v in the neon sequence
Author:
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevA.37.1872/fulltext
Reference17 articles.
1. Techniques for the calculation of atomic structures and radiative data including relativistic corrections
2. The 2s3p3P1-2s21S0intercombination line in the beryllium sequence
3. Some O I oscillator strengths and the interstellar abundance of oxygen
4. A correction method for fine-structure calculations: application to neon 3p J=2 levels
5. A correction method for fine-structure calculations. II. Application to neon 3s and 3p excited levels
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1. Semiempirical calculation of the fine-structure parameters for np 5 n′p configurations;Optics and Spectroscopy;2000-03
2. Transition probabilities for 3p→3s and 3d→3p lines of NaII;Journal of Quantitative Spectroscopy and Radiative Transfer;1993-07
3. Oscillator strengths for transitions among sextet states in Cr II;Physica Scripta;1990-08-01
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