[1] We discuss that energetic electrons are generated near the X-type magnetic reconnection region due to a surfing acceleration mechanism. In a thin plasma sheet the polarization electric fields pointing toward the neutral sheet are induced around the boundary between the lobe and plasma sheet in association with the Hall electric current. By using a particle-in-cell simulation, we demonstrate that the polarization electric fields are strongly enhanced in an externally driven reconnection system, and some electrons can be trapped by the electrostatic potential well of the polarization field. During the trapping phase the electrons can gain their energies from the convection/inductive reconnection electric fields. We discuss that relativistic electrons with MeVenergies are quickly generated in and around the X-type neutral region by utilizing the surfing acceleration. Copyright 2005 by the American Geophysical Union.
Mendeley helps you to discover research relevant for your work.
CITATION STYLE
Hoshino, M. (2005). Electron surfing acceleration in magnetic reconnection. Journal of Geophysical Research: Space Physics, 110(A10). https://doi.org/10.1029/2005JA011229