Non-thermal Acceleration from Reconnection Shocks
arXiv:astro-ph/9410036 · doi:10.1103/PhysRevLett.73.3097
Abstract
Reconnection shocks in a magnetically dominated plasma must be compressive. Non-thermal ion acceleration can occur across built-in slow shocks, and across outflow fast shocks when the outflow is supermagnetosonic and the field is line-tied. Electron acceleration may be initiated by injection from the dissipation region. Reconnection and shock acceleration thus cooperate and non-thermal acceleration should be a characteristic feature.
12 pages, plain TeX, accepted for publication in Phys. Rev. Lett
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