Magnetic reconnection configurations and particle acceleration in solar flares |
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| Institution: | Department of Astronomy, Nanjing University, Nanjing 210093, China |
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| Abstract: | Numerical simulations of two types of flares indicate that magnetic reconnection can provide environments favorable for various particle acceleration mechanisms to work. This paper reviews recent test particle simulations of DC electric field mechanism, and discusses how the flare particles can escape into the interplanetary space under different magnetic configurations. |
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