For pt.I see ibid., vol.8, no.23, p.4124 (1975). The low-energy satellites of K beta 1,3 lines of metallic Co, Ni, Cu, and Zn have been measured. These spectra are interpreted in terms of the K to M 2 radiative Auger (RA) effect because the energies of the satellite edges are in accordance with Auger electron observation and the intensities compare favourably with the theoretical RA shake-off calculation. The intensities of interfering lines due to resonant Raman, K alpha h hypersatellite, and radiative rearrangement (RER) transitions, are found to be negligible in comparison with RA intensity in the whole period 15
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Keski‐Rahkonen et al. (1980) studied this question.
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