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Oscillator strengths for 2pnd−2pn′f transitions of Ci and identifications in the infrared solar photospheric spectrum (1 ≤ λ ≤ 3μ)

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Abstract

Absolute transition probabilities are calculated for 2p(2 P) nd − 2p(2 P) n′f transitions of Ci (1 ⩽ λ ⩽ 3μ). Pair coupling expressions for line strengths are used and the radial wavefunctions are obtained through the use of the Coulomb approximation.

A description of the occurrence of these lines in the solar photospheric spectrum is presented and 47 new identifications are proposed.

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  1. Institut d'Astrophysique, Université de Liège, B-4200/Cointe-Ougrée, Belgique

    E. Biémont

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  1. E. Biémont
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Biémont, E. Oscillator strengths for 2pnd−2pn′f transitions of Ci and identifications in the infrared solar photospheric spectrum (1 ≤ λ ≤ 3μ). Sol Phys 32, 117–129 (1973). https://doi.org/10.1007/BF00152732

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  • DOI: https://doi.org/10.1007/BF00152732

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