Figure 11
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>70 MeV proton fluxes in year 2020 (solar minimum) and year 2024 (approximately solar maximum) at POES altitude. upper row: POES observations; second row: simulations by the new method; third row: simulations by IRENE-AP9 (V1.57, mean mode); forth row: simulation by AP8-MIN and AP8-MAX, with geomagnetic field shifting (5° N, 15° W) to match the flux peak location; bottom row: scatter plots to compare model simulations with POES observations.
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