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 |
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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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