Numerical simulations indicate that particle scattering in anisotropic turbulence without a guide field is independent of correlation length and follows a mechanism distinct from pitch-angle diffusion.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Observed CR pitch-angle diffusion matches quasi-slab fast-mode turbulence predictions shaped by damping, but not Alfvénic turbulence, evidencing fast-mode dominance and constraining LISM to low beta ≈0.1 with δB/B0 ≈0.5.
Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.
citing papers explorer
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High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields
Numerical simulations indicate that particle scattering in anisotropic turbulence without a guide field is independent of correlation length and follows a mechanism distinct from pitch-angle diffusion.