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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