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arXiv · astro-ph/9410036

Non-thermal Acceleration from Reconnection Shocks

Eric G. Blackman·George B. Field
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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.

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Eric G. Blackman, George B. Field. 1994-10-12. Non-thermal Acceleration from Reconnection Shocks. https://doi.org/10.1103/physrevlett.73.3097

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