Magnetic Reconnection

Masaaki Yamada, Russell Kulsrud and Hantao Ji

关键词: DOCUMENTATION;    MAGNETIC RECONNECTION;    PLASMA;    THERMONUCLEAR REACTIONS;    ASTROPHYSICS Magnetic Self-organization;    Laboratory Astrophysics;    Magnetic Reconnection;   

DOI  :  10.2172/965275
RP-ID  :  PPPL-4457
PID  :  OSTI ID: 965275
Others  :  TRN: US0903848

美国|英语

来源: SciTech Connect

【 摘 要 】

We review the fundamental physics of magnetic reconnection in laboratory and space plasmas, by discussing results from theory, numerical simulations, observations from space satellites, and the recent results from laboratory plasma experiments. After a brief review of the well-known early work, we discuss representative recent experimental and theoretical work and attempt to interpret the essence of significant modern findings. In the area of local reconnection physics, many significant findings have been made with regard to two- uid physics and are related to the cause of fast reconnection. Profiles of the neutral sheet, Hall currents, and the effects of guide field, collisions, and micro-turbulence are discussed to understand the fundamental processes in a local reconnection layer both in space and laboratory plasmas. While the understanding of the global reconnection dynamics is less developed, notable findings have been made on this issue through detailed documentation of magnetic self-organization phenomena in fusion plasmas. Application of magnetic reconnection physics to astrophysical plasmas is also brie y discussed.