Magnetic Field Line Random Walk and Solar Energetic Particle Path Lengths: Stochastic Theory and PSP/ISoIS Observation
R. Chhiber,W. H. Matthaeus, C. M. S. Cohen,D. Ruffolo,W. Sonsrettee,P. Tooprakai,A. Seripienlert,P. Chuychai,A. Usmanov,M. L. Goldstein, D. J. McComas, R. A. Leske,J. R. Szalay,C. J. Joyce, A. C. Cummings,E. C. Roelof, E. R. Christian, R. A. Mewaldt, A. W. Labrador,J. Giacalone, N. A. Schwadron, D. G. Mitchell,M. E. Hill, M. E. Wiedenbeck, R. L. McNutt, M. Desai arXiv (Cornell University)(2020)
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turbulence,solar wind,Sun,magnetic fields,diffusion,Sun,flares,acceleration of particles
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