4.4 Article

Electron acceleration in three-dimensional magnetic reconnection with a guide field

期刊

PHYSICS OF PLASMAS
卷 22, 期 10, 页码 -

出版社

AIP Publishing
DOI: 10.1063/1.4933212

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资金

  1. NSF [AGS1202330, PHY1102479]
  2. NASA [NNX11AQ93H, APL-975268, NNX08AV87G, NAS 5-98033, NNX08AO83G]
  3. Directorate For Geosciences
  4. Div Atmospheric & Geospace Sciences [1202330] Funding Source: National Science Foundation
  5. Division Of Physics
  6. Direct For Mathematical & Physical Scien [1337831] Funding Source: National Science Foundation
  7. NASA [94116, NNX08AV87G, NNX11AQ93H, 139034] Funding Source: Federal RePORTER

向作者/读者索取更多资源

Kinetic simulations of 3D collisionless magnetic reconnection with a guide field show a dramatic enhancement of energetic electron production when compared with 2D systems. In the 2D systems, electrons are trapped in magnetic islands that limit their energy gain, whereas in the 3D systems the filamentation of the current layer leads to a stochastic magnetic field that enables the electrons to access volume-filling acceleration regions. The dominant accelerator of the most energetic electrons is a Fermi-like mechanism associated with reflection of charged particles from contracting field lines. (C) 2015 AIP Publishing LLC.

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