Dynamic modeling of the Earth’s trapped proton environment | Journal of Space Weather and Space Climate

Open Access

Figure S4.

Model calculated >70 MeV proton fluxes (with g_h function and H_min(L, α_m)=100 km, optimal collisional loss coefficients: a = 17.5, z₁ = −50 km, z₂ = 0.351, b= 1.142), and their comparisons with the observations by RPS-b (2013) and SEM2/POES (1998–2013). The figures are similar to Figures 6–9.

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