磁拓扑是在等离子物理学中,其等离子的磁场结构和联系[1][2]

等离子的磁拓扑可以通过磁扩散英语Magnetic diffusion重联来改变。然而,在大磁雷诺数的极限下,磁场的扩散和重联不可能发生,因而磁拓扑结构得以保留[3][4]

参考资料

编辑
  1. ^ Longcope, Dana W. Topological Methods for the Analysis of Solar Magnetic Fields. Living Reviews in Solar Physics. 2005, 2. doi:10.12942/lrsp-2005-7. 
  2. ^ Hornig, G.; Schindler, K. Magnetic topology and the problem of its invariant definition. Physics of Plasmas. March 1996, 3 (3): 781–791. doi:10.1063/1.871778. 
  3. ^ Gonzalez, Walter; Parker, Eugene (编). Magnetic reconnection: concepts and applications. Cham: Springer. 2016. ISBN 978-3-319-26432-5. 
  4. ^ Parker, E. N. Cosmical magnetic fields: their origin and their activity. Oxford: Clarendon Press. 1979. ISBN 0198512902. 

Template:Plasma-stub