磁拓撲是在等離子物理學中,其等離子的磁場結構和聯繫[1][2]

等離子的磁拓撲可以通過磁擴散英語Magnetic diffusion重聯來改變。然而,在大磁雷諾數的極限下,磁場的擴散和重聯不可能發生,因而磁拓撲結構得以保留[3][4]

參考資料

  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 (編). 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