Impact of solar magnetic field amplitude and geometry on cosmic rays diffusion coefficients in the inner heliosphere | Journal of Space Weather and Space Climate

Topical Issue - Space climate: The past and future of solar activity

Open Access

Fig. 5

Meridional cuts of the parallel mfp λ_|| and the perpendicular mfp λ_⊥ in AU for a proton of rigidity 445 MV (which means 100 MeV energy). The two panels on the left correspond to the case D1, the two panels on the right correspond to the case Q1.

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