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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.
citing papers explorer
-
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.
-
Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies
Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.