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. Author manuscript; available in PMC: 2021 Oct 27.
Published in final edited form as: Astrophys J. 2017 May 15;840(2):115. doi: 10.3847/1538-4357/aa6e4f

Figure 9.

Figure 9.

Antiproton differential intensities for 2007 December (BESS; left) and averaged for 2006–2009 (PAMELA; right). Circles represent experimental data, the dashed line is the GALPROP LIS, and the solid line is the computed modulated spectrum. The bottom panel is the relative difference between the numerical solution and experimental data.