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Electron acceleration in reconnecting current sheets View all abstracts by submitter

Thomas Neukirch   Submitted: 2004-09-23 07:35

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.

Authors: Wood, P. and Neukirch, T.
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Publication Status: Solar Physics (accepted)
Last Modified: 2004-10-24 14:23
Go to main E-Print page  Reconstruction of a Magnetohydrodynamic Velocity Field Vector 
from Doppler Motions and a Pair of Solar Vector Magnetograms  PHYSICS OF THE SOLAR CORONA. AN INTRODUCTION  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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