Abstract
Most of the atomic processes described in this book by the other contributors will eventually lead to the emission of photons by excited atoms. Whether these photons are considered as beneficial — for diagnostic purposes, or detrimental — causing energy losses, is not our concern here. In either case, however, control of the plasma requires the knowledge of the ratio of the number of photons corresponding to a given transition emitted per unit time from an excited state to the number of atoms lying in the excited state, per unit volume. This defines the transition probability (abbreviated below as TP). Let us recall also that oscillator strengths, (OS) defined below, are needed in the estimation of collision excitation cross sections by semi empirical formulas — which will probably continue to be widely used for a long time.
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Klapisch, M. (1980). Theoretical Studies of Oscillator Strengths for the Spectroscopy of Hot Plasmas. In: McDowell, M.R.C., Ferendeci, A.M. (eds) Atomic and Molecular Processes in Controlled Thermonuclear Fusion. NATO Advanced Study Institutes Series, vol 53. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-9161-0_14
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