Abstract

Hartree–Fock calculations have been performed for Ne vi, Al ix, Si x, S xii, Ar xiv, and Fe xxii. Spin– orbit interaction and configuration interaction, particularly (2s2 2p+2p3)2P, have been included to obtain energy levels and transition probabilities for the array (2s2 2p+2p3) → (2s2p2+2s2 nl) with n = 3 and 4 and l = 0, 1, and 2.

© 1971 Optical Society of America

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