Simulations show mirror diffusion confines cosmic rays more than scattering during the superdiffusive phase, with fitted mean-free-path scalings λ∥∝Rg^{1/3}, λ⊥∝Rg^{2/3} in sub-Alfvénic turbulence and mode-specific dominance for parallel and perpendicular transport.
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Studying the diffusion mechanism of cosmic-ray particles
Simulations show mirror diffusion confines cosmic rays more than scattering during the superdiffusive phase, with fitted mean-free-path scalings λ∥∝Rg^{1/3}, λ⊥∝Rg^{2/3} in sub-Alfvénic turbulence and mode-specific dominance for parallel and perpendicular transport.