Volume 574, February 2015
|Number of page(s)||15|
|Published online||16 January 2015|
Particle acceleration at a reconnecting magnetic separator
School of Mathematics and Statistics, University of St Andrews, St Andrews, Fife KY16 9SS, UK
e-mail: email@example.com; firstname.lastname@example.org; email@example.com; firstname.lastname@example.org
Received: 10 June 2014
Accepted: 22 October 2014
Context. While the exact acceleration mechanism of energetic particles during solar flares is (as yet) unknown, magnetic reconnection plays a key role both in the release of stored magnetic energy of the solar corona and the magnetic restructuring during a flare. Recent work has shown that special field lines, called separators, are common sites of reconnection in 3D numerical experiments. To date, 3D separator reconnection sites have received little attention as particle accelerators.
Aims. We investigate the effectiveness of separator reconnection as a particle acceleration mechanism for electrons and protons.
Methods. We study the particle acceleration using a relativistic guiding-centre particle code in a time-dependent kinematic model of magnetic reconnection at a separator.
Results. The effect upon particle behaviour of initial position, pitch angle, and initial kinetic energy are examined in detail, both for specific (single) particle examples and for large distributions of initial conditions. The separator reconnection model contains several free parameters, and we study the effect of changing these parameters upon particle acceleration, in particular in view of the final particle energy ranges that agree with observed energy spectra.
Key words: plasmas / Sun: corona / Sun: magnetic fields / Sun: activity / acceleration of particles
© ESO, 2015
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