Shocks and Waves
Apr 27, 2020
Prof. Bin Chen
Solar Astrophysicist
Professor of Physics
My research interests include radio astronomy and instrumentation, solar flares, coronal mass ejections, magnetic reconnection, shocks, and particle acceleration.
Related
Publications
Solar flare termination shocks have been suggested as one of the viable mechanisms for accelerating electrons and ions to high …
Yingjie Luo,
Bin Chen,
Sijie Yu,
T. Bastian,
Säm Krucker
Nonthermal loop-top sources in solar flares are the most prominent observational signatures that suggest energy release and particle …
Xiangliang Kong,
Fan Guo,
Chengcai Shen,
Bin Chen,
Yao Chen,
Sophie Musset,
Lindsay Glesener,
Peera Pongkitiwanichakul,
Joe Giacalone
Solar flare termination shocks have been suggested as one of the promising drivers for particle acceleration in solar flares, yet …
Bin Chen,
Chengcai Shen,
Katharine K. Reeves,
Fan Guo,
Sijie Yu
Solar flares involve the sudden release of magnetic energy in the solar corona. Accelerated nonthermal electrons have often been …
Sijie Yu,
Bin Chen
In eruptive solar flares, termination shocks (TSs), formed when high- speed reconnection outflows collide with closed dense flaring …
Chengcai Shen,
Xiangliang Kong,
Fan Guo,
John C. Raymond,
Bin Chen
An observation from the Interface Region Imaging Spectrograph reveals coherent oscillations in the loops of an M1.6 flare on 2015 March …
Hui Tian,
Peter R. Young,
Katharine K. Reeves,
Tongjiang Wang,
Patrick Antolin,
Bin Chen,
Jiansen He
Solar flares—the most powerful explosions in the solar system—are also efficient particle accelerators, capable of energizing a large …
Bin Chen,
Timothy S. Bastian,
Chengcai Shen,
Dale E. Gary,
Säm Krucker,
Lindsay Glesener