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Magnetic reconnection configurations and particle acceleration in solar flares.
| Content Provider | CiteSeerX |
|---|---|
| Author | Chen, P. F. Liu, W. J. Fang, C. |
| 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. Key words: solar flares, magnetic reconnection, particle acceleration |
| File Format | |
| Access Restriction | Open |
| Subject Keyword | Solar Flare Particle Acceleration Magnetic Reconnection Configuration Magnetic Reconnection Numerical Simulation Different Magnetic Configuration Dc Electric Field Mechanism Key Word Interplanetary Space Flare Particle Various Particle Acceleration Mechanism Recent Test Particle Simulation |
| Content Type | Text |
| Resource Type | Article |