Space Science Reviews

, Volume 172, Issue 1–4, pp 283–302

Magnetic Reconnection for Coronal Conditions: Reconnection Rates, Secondary Islands and Onset



Magnetic reconnection may play an important role in heating the corona through a release of magnetic energy. An understanding of how reconnection proceeds can contribute to explaining the observed behavior. Here, recent theoretical work on magnetic reconnection for coronal conditions is reviewed. Topics include the rate that collisionless (Hall) reconnection proceeds, the conditions under which Hall reconnection begins, and the effect of secondary islands (plasmoids) both on the scaling and properties of collisional (Sweet-Parker) reconnection and on the onset of Hall reconnection. Applications to magnetic energy storage and release in the corona are discussed.


Magnetic reconnection Collisionless reconnection Hall reconnection Secondary Islands Plasmoids Solar corona 


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Copyright information

© Springer Science+Business Media B.V. 2011

Authors and Affiliations

  1. 1.Department of PhysicsWest Virginia UniversityMorgantownUSA
  2. 2.Department of Physics and AstronomyUniversity of DelawareNewarkUSA

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