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Calculated Auger, Coster-Kronig, super Coster-Kronig, and radiative transition rates are used to compute atomic M-shell Auger, Coster-Kronig, and fluorescence yields. Comparison is made with five fluorescence-field measurements, with full width at half-maximum measurements of L-M x rays, and with Bhalla's relativistic radiative-yield calculations.
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E. J. McGuire (1972) studied this question.
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