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Chengcai Shen
Harvard-Smithsonian Center for AstrophysicsMeeting roles in:
Particle Acceleration and Transport in 3D Solar Flare Simulations
Modeling Fast Magnetic Reconnection in Solar Flare Current Sheets
Evolution of solar wind charge states from the solar corona to 1 AU with nonthermal electrons
Unveiling the nature of non-thermal coronal sources in eruptive solar flares using model-to-data comparisons
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