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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Main Authors: W. Sonsrettee, P. Subedi, D. Ruffolo, W. H. Matthaeus, A. P. Snodin, P. Wongpan, P. Chuychai
其他作者: Mahidol University
格式: Article
出版: 2018
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在線閱讀:https://repository.li.mahidol.ac.th/handle/123456789/35891
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機構: Mahidol University

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