Space Science Reviews

, Volume 173, Issue 1–4, pp 223–245 | Cite as

Current Fragmentation and Particle Acceleration in Solar Flares

  • P. J. Cargill
  • L. Vlahos
  • G. Baumann
  • J. F. Drake
  • Å. Nordlund
Article

Abstract

Particle acceleration in solar flares remains an outstanding problem in plasma physics and space science. While the observed particle energies and timescales can perhaps be understood in terms of acceleration at a simple current sheet or turbulence site, the vast number of accelerated particles, and the fraction of flare energy in them, defies any simple explanation. The nature of energy storage and dissipation in the global coronal magnetic field is essential for understanding flare acceleration. Scenarios where the coronal field is stressed by complex photospheric motions lead to the formation of multiple current sheets, rather than the single monolithic current sheet proposed by some. The currents sheets in turn can fragment into multiple, smaller dissipation sites. MHD, kinetic and cellular automata models are used to demonstrate this feature. Particle acceleration in this environment thus involves interaction with many distributed accelerators. A series of examples demonstrate how acceleration works in such an environment. As required, acceleration is fast, and relativistic energies are readily attained. It is also shown that accelerated particles do indeed interact with multiple acceleration sites. Test particle models also demonstrate that a large number of particles can be accelerated, with a significant fraction of the flare energy associated with them. However, in the absence of feedback, and with limited numerical resolution, these results need to be viewed with caution. Particle in cell models can incorporate feedback and in one scenario suggest that acceleration can be limited by the energetic particles reaching the condition for firehose marginal stability. Contemporary issues such as footpoint particle acceleration are also discussed. It is also noted that the idea of a “standard flare model” is ill-conceived when the entire distribution of flare energies is considered.

Keywords

Solar flares 

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Copyright information

© Springer Science+Business Media B.V. 2012

Authors and Affiliations

  • P. J. Cargill
    • 1
    • 2
  • L. Vlahos
    • 3
  • G. Baumann
    • 4
  • J. F. Drake
    • 5
  • Å. Nordlund
    • 4
  1. 1.Space and Atmospheric Physics, The Blackett LaboratoryImperial CollegeLondonUK
  2. 2.School of Mathematics and StatisticsUniversity of St AndrewsSt AndrewsUK
  3. 3.Department of PhysicsAristotle University of ThessalonikiThessalonikiGreece
  4. 4.Niels Bohr InstituteUniversity of CopenhagenCopenhagenDenmark
  5. 5.Institute for Research in Electronics and Applied PhysicsUniversity of MarylandCollege ParkUSA

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