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. Author manuscript; available in PMC: 2021 Oct 27.
Published in final edited form as: Astrophys J Suppl Ser. 2020 Sep 29;250(2):27. doi: 10.3847/1538-4365/aba901

Figure 1.

Figure 1.

Calculated elemental spectra: 2He–10Ne. Black dashed lines show the calculated LIS spectra; the red solid lines are modulated to the levels that correspond to the periods of data taking. Data for Z ⩾ 4: ACE-CRIS and HEAO-3-C2 (Engelmann et al. 1990). AMS-02 data for 2He and 3Li are compared to the I-scenario calculations; see Section 3.2 for details. Bottom panels in each plot show the relative difference between the calculations and a corresponding data set.