Particle dynamics in a non-flaring solar active region model

J. Threlfall, Ph A. Bourdin, T. Neukirch, C. E. Parnell

Research output: Contribution to journalArticlepeer-review

12 Citations (Scopus)


Aims. The aim of this work is to investigate and characterise particle behaviour in an (observationally-driven) 3D magnetohydrodynamic (MHD) model of the solar atmosphere above a slowly evolving, non-flaring active region. Methods. We use a relativistic guiding-centre particle code to investigate the behaviour of selected particle orbits, distributed throughout a single snapshot of the 3D MHD simulation. Results. Two distinct particle acceleration behaviours are recovered, which affect both electrons and protons: (i) direct acceleration along field lines and (ii) tangential drifting of guiding centres with respect to local magnetic field. However, up to 40% of all particles actually experience a form of (high energy) particle trap, because of changes in the direction of the electric field and unrelated to the strength of the magnetic field; such particles are included in the first category. Additionally, category (i) electron and proton orbits undergo surprisingly strong acceleration to non-thermal energies (≠42 MeV), because of the strength and extent of super-Dreicer electric fields created by the MHD simulation. Reducing the electric field strength of the MHD model does not significantly affect the efficiency of the (electric field-based) trapping mechanism, but does reduce the peak energies gained by orbits. We discuss the implications for future experiments, which aim to simulate non-flaring active region heating and reconnection.

Original languageEnglish
Article numberA4
Number of pages13
JournalAstronomy and Astrophysics
Early online date11 Feb 2016
Publication statusPublished - 1 Mar 2016
Externally publishedYes


  • Plasmas
  • Sun: corona
  • Sun: magnetic fields
  • Sun: activity
  • Acceleration of particles


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