Fig. 3.

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Cosmic rays in the solar neighborhood. Upper panel: Model CR particle density spectra. Middle panel: CR energy spectra. The solid black line shows the CR electron model (Pohl 1993), the solid red line shows the CR proton model (Pohl 1993), the solid blue line shows the GALPROP model fit to observations by Cummings et al. (2016), and triangles shows Voyager 1 data (Cummings et al. 2016) and AMS data (Aguilar et al. 2019). Lower panel: CR injection spectra.
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