Solar Physics

, Volume 226, Issue 1, pp 73–95 | Cite as

Electron Acceleration in Reconnecting Current Sheets

  • Paul Wood
  • Thomas Neukirch


We present the results of charged particle orbit calculations in prescribed electric and magnetic fields motivated by magnetic reconnection models. Due to the presence of a strong guide field, the particle orbits can be calculated in the guiding centre approximation. The electromagnetic fields are chosen to resemble a reconnecting magnetic current sheet with a localised reconnection region. An initially Maxwellian distribution function in the inflow region can develop a beam-like component in the outflow region. Possible implications of these findings for acceleration scenarios in solar flares will be discussed.


Flare Current Sheet Solar Flare Magnetic Reconnection Electron Acceleration 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer Science + Business Media, Inc. 2005

Authors and Affiliations

  1. 1.School of Mathematics and StatisticsUniversity of St. AndrewsSt. AndrewsU.K.

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