Fig. 6.

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Energy-per-nucleon spectra at ωcpt = 48.99. The original spectra of different ion species (a) and spectra of heavy ions shifted for visibility on the y-axis by a factor of 100, 101, 102, and 103 for 4He2+, 3He2+, 16O7+, and 56Fe14+, respectively (b). The dashed lines in the right panel are the power-law fit (Eγ) to the shoulder region of the spectra, where E is the energy-per-nucleon.
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