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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Numerical tracing of stochastic Parker spirals yields an angular field line spread of ~25° at 1 AU that narrows to ~4° when integrated backward to the solar source surface at 0.25 AU.
A systematic comparison finds that direction-averaging shows polar and azimuthal dependence but is insensitive to spacecraft configuration, while lag polyhedral derivative ensemble is strongly affected by spacecraft separation and shape but insensitive to sampling trajectory.
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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.