Abstract
We employ a test-particle code to explore diffusion of energetic particles interacting with the solar wind plasma.The first time we investigate the pitch-angle dependence of perpendicular diffusion for different parameter regimes.These results are important for numerical solutions of the pitch-angle dependent Cosmic Ray Fokker-Planck equa-tion. We compare our finding also with predictions made by analytical theory.
Cite
CITATION STYLE
Qin, G., & Shalchi, A. (2013). Pitch-Angle Dependent Perpendicular Diffusion of Energetic Particles Interacting With Magnetic Turbulence. Applied Physics Research, 6(1). https://doi.org/10.5539/apr.v6n1p1
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