Magnetic field line random walk in isotropic turbulence with zero mean field

© 2015. The American Astronomical Society. All rights reserved. In astrophysical plasmas, magnetic field lines often guide the motions of thermal and non-thermal particles. The field line random walk (FLRW) is typically considered to depend on the Kubo number R = (b/B0)(ℓ∥/ℓ⊥) for rms magnetic fluct...

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Bibliographic Details
Main Authors: W. Sonsrettee, P. Subedi, D. Ruffolo, W. H. Matthaeus, A. P. Snodin, P. Wongpan, P. Chuychai
Other Authors: Mahidol University
Format: Article
Published: 2018
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Online Access:https://repository.li.mahidol.ac.th/handle/123456789/35891
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Institution: Mahidol University

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