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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 7.

Figure 7.

GalProp source and LIS abundances for elements Z = 1–28 at 100 MeV nucleon−1 and 10 GeV nucleon−1 w.r.t. silicon (Si = 100) in our model. The abundances are tuned to Voyager 1 data (Cummings et al. 2016) and the HEAO-3-C2 “plateau” region (Engelmann et al. 1990).