“…For the K h α hypersatellite lines, in particular, in the case of 3 d transition metals, such discrepancies have been already observed (see, e.g.,the studies of Hoszowska et al and Diamant et al). From the reported K h β 1,3 hypersatellite spectra plots for Sc, Ti, and Fe, one can derive FWHM widths of about 7, 8, and 15 eV, respectively. The FWHM of Sc (Z=21) and Ti (Z=22) are comparable with the FWHM of 8.8 eV obtained in this work for Cr (Z=24), whereas the value found for Fe (Z=26) seems to be unexpectedly high as compared with those of the three lighter elements.…”