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Figure 9
NRR time spectra calculated for several grazing angles for two models of hyperfine field depth distribution: (a) for the model obtained by fitting of the experimental data at the position irradiated with a fluence of 0.75 × 1014 ions cm−2 and (b) for the same case but with homogeneously distributed hyperfine fields across the film depth.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 28| Part 5| September 2021| Pages 1535-1543
https://doi.org/10.1107/S1600577521007694
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