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Cited article:

Magnetic field line random walk in two-dimensional dynamical turbulence

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Parallel and perpendicular diffusion coefficients of energetic particles interacting with shear Alfvén waves

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Monthly Notices of the Royal Astronomical Society 444 (3) 2676 (2014)
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Magnetic correlation functions in the slow and fast solar wind in the Eulerian reference frame

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Compound diffusion of energetic particles: a Kappa model for the parallel distribution function

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Astrophysics and Space Science 340 (2) 351 (2012)
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Random walk of magnetic field lines in dynamical turbulence: A field line tracing method. II. Two-dimensional turbulence

B. Guest and A. Shalchi
Physics of Plasmas 19 (3) (2012)
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A heuristic derivation of an improved analytical theory for perpendicular diffusion of charged particles

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Advances in Space Research 48 (9) 1499 (2011)
https://doi.org/10.1016/j.asr.2011.07.016

Simulating heliospheric and solar particle diffusion using the Parker spiral geometry

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Journal of Geophysical Research: Space Physics 116 (A2) n/a (2011)
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Random walk of magnetic field lines in dynamical turbulence: A field line tracing method. I. Slab turbulence

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Compound and perpendicular diffusion of cosmic rays and random walk of the field lines: II. Non-parallel particle transport and drifts

G M Webb, E Kh Kaghashvili, J A le Roux, et al.
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https://doi.org/10.1088/1751-8113/42/23/235502

Compound perpendicular transport of charged particles with drift, advection, wave propagation effects, and an arbitrary turbulence spectrum

A. Shalchi, G. M. Webb, J. A. le Roux and G. P. Zank
Astrophysics and Space Science 321 (3-4) 197 (2009)
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