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Cited article:

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Turbulent Origins of Particle Intensity Dropout in Gradual Solar Energetic Particle Events During Solar Cycle 23

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Energetic Particle Superdiffusion in Solar System Plasmas: Which Fractional Transport Equation?

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Detailed test-particle simulations of energetic particles interacting with magnetized plasmas I. Two-component turbulence

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Non-Markovian Pitch-angle Scattering as the Origin of Particle Superdiffusion Parallel to the Magnetic Field

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Subspace approximations to the cosmic ray Fokker–Planck equation

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Pitch-angle Diffusion and Bohm-type Approximations in Diffusive Shock Acceleration

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Parallel and Perpendicular Diffusion Coefficients of Energetic Charged Particles with Adiabatic Focusing

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Time-dependent transport of energetic particles in magnetic turbulence: computer simulations versus analytical theory

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Numerical analysis of the Fokker-Planck equation with adiabatic focusing: Realistic pitch-angle scattering

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Time-dependent Perpendicular Transport of Energetic Particles for Different Turbulence Configurations and Parallel Transport Models

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Cosmic-ray diffusion modeling: Solutions using variational methods

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The Astrophysical Journal 720 (2) L127 (2010)
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Analytical description of nonlinear cosmic ray scattering: isotropic and quasilinear regimes of pitch-angle diffusion

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Aspects of self-similar current distributions resulting from the plasma filamentation instability

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Comparison between test-particle simulations and test-particle theories for cosmic ray transport: I. Magnetostatic turbulence

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Journal of Physics G: Nuclear and Particle Physics 32 (6) 809 (2006)
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