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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 3.

Figure 3.

GalProp–HelMod LIS and modulated spectra are compared with AMS-02 data for 10Ne, 12Mg, and 14Si (Aguilar et al. 2020). Shown are the calculations made in the I-scenario. The lower panels show the relative difference in two ways: AMS-02-data-centered as in our previous papers, and in a more traditional model-prediction-centered view. Line coding is the same as in Figure 1.