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An Evaluation of Different Numerical Methods to Calculate the Pitch-angle Diffusion Coefficient from Full-orbit Simulations: Disentangling a Rope of Sand
Cloud-scale radio surveys of star formation and feedback in Triangulum Galaxy M 33: VLA observations
F S Tabatabaei, W Cotton, E Schinnerer, et al. Monthly Notices of the Royal Astronomical Society 517(2) 2990 (2022) https://doi.org/10.1093/mnras/stac2514
A Comparison with Theory of Computation and Estimation of Pitch-Angle Diffusion Coefficients from Simulations in Noisy Reduced Magnetohydrodynamic Turbulence
THE DIFFUSION APPROXIMATION VERSUS THE TELEGRAPH EQUATION FOR MODELING SOLAR ENERGETIC PARTICLE TRANSPORT WITH ADIABATIC FOCUSING. I. ISOTROPIC PITCH-ANGLE SCATTERING