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Figure 4.
Fluorescence and Auger electron yields as a function of atomic number for K shell vacancies.
Auger transitions ( red curve ) are more probable for lighter elements, while X-ray yield ( dotted blue curve ) becomes dominant at higher atomic numbers.
Similar plots can be obtained for L and M shell transitions.
Coster – Kronig ( i. e. intra-shell ) transitions are ignored in this analysis.

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