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Open Issues in Non-Gaussian Transport and Acceleration of Charged Energetic Particles in Space and Astrophysical Plasmas
F. Effenberger, D. Walter, H. Fichtner, S. Aerdker, R. Grauer, T. Laitinen, J. A. le Roux, Y. Litvinenko, J. Lübke, S. Perri, P. Reichherzer, A. Shalchi, J. P. van den Berg and G. Zimbardo Space Science Reviews 221(5) (2025) https://doi.org/10.1007/s11214-025-01203-4
An Evaluation of Different Numerical Methods to Calculate the Pitch-angle Diffusion Coefficient from Full-orbit Simulations: Disentangling a Rope of Sand
A Comparison with Theory of Computation and Estimation of Pitch-Angle Diffusion Coefficients from Simulations in Noisy Reduced Magnetohydrodynamic Turbulence
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
Non-Markovian Pitch-angle Scattering as the Origin of Particle Superdiffusion Parallel to the Magnetic Field
THE DIFFUSION APPROXIMATION VERSUS THE TELEGRAPH EQUATION FOR MODELING SOLAR ENERGETIC PARTICLE TRANSPORT WITH ADIABATIC FOCUSING. I. ISOTROPIC PITCH-ANGLE SCATTERING