Fig. 8.

3He/4He as a function of Ek/n for AMS-02 (purple squares) and PAMELA (green crosses)–the latter combine data from two different analysis, respectively PAMELA-ToF and PAMELA-Calorimeter (Adriani et al. 2016). All models are calculated from the best-fit parameters of the combined analysis of Li/C, Be/C, B/C, N/O, 3He, and 4He AMS-02 data. Different line styles show different model configurations (BIG, SLIM, and QUAINT) and their respective post-fit solar modulation level in purple. Green lines show the same model calculations but modulated at the PAMELA expected value of 539 MV.
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