Magnetic Reconnection
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
As one of the most spectacular energy release events in the solar system, solar flares are generally powered by magnetic reconnection …
T. Samanta,
H. Tian,
B. Chen,
K. Reeves,
M. Cheung,
A. Vourlidas,
D. Banerjee
A fast-mode shock can form in the front of reconnection outflows and has been suggested as a promising site for particle acceleration …
Xiangliang Kong,
Fan Guo,
Chengcai Shen,
Bin Chen,
Yao Chen,
Joe Giacalone
In this study, we investigate motions in the hot plasma above the flare loops during the 2017 September 10 X8.2 flare event. We examine …
Katharine K. Reeves,
Vanessa Polito,
Bin Chen,
Giselle Galan,
Sijie Yu,
Wei Liu,
Gang Li
Magnetic reconnection plays a crucial role in powering solar flares, production of energetic particles, and plasma heating. However, …
Sijie Yu,
Bin Chen,
Katharine K. Reeves,
Dale E. Gary,
Sophie Musset,
Gregory D. Fleishman,
Gelu M. Nita,
Lindsay Glesener
In the standard model of solar flares, a large-scale reconnection current sheet is postulated to be the central engine for powering the …
Bin Chen,
Chengcai Shen,
Dale E. Gary,
Katharine K. Reeves,
Gregory D. Fleishman,
Sijie Yu,
Fan Guo,
Säm Krucker,
Jun Lin,
Gelu M. Nita,
Xiangliang Kong
Jets are ubiquitously present in both quiet and active regions on the Sun. They are widely believed to be driven by magnetic …
Zhicheng Zeng,
Bin Chen,
Haisheng Ji,
Philip R. Goode,
Wenda Cao
Magnetic reconnection is believed to be the dominant energy release mechanism in solar flares. The standard flare model predicts both …
Hui Tian,
Gang Li,
Katharine K. Reeves,
John C. Raymond,
Fan Guo,
Wei Liu,
Bin Chen,
Nicholas A. Murphy