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Figure 3
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y, >70 MeV proton flux observations normalized to feq(L), as a function of B/B0 in six L shells of the IGRF field for year 2013. Discrete data points: based on observations by RPS-b at high altitudes (Hmin > 1000 km) in year 2013; Solid line: gb function, computed with value of k indicated (see Eq. (6)).
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