Dr. Bin Chen is a Professor of Physics at the New Jersey Institute of Technology. Research in his group focuses on solar flares and coronal mass ejections, the largest explosions in the solar system that can affect our Earth and near-Earth environment, known as Space Weather. He develops novel radio observing techniques and utilizes multi-wavelength observations to study physical processes underlying these catastrophic energy release events. He co-leads the NJIT solar radio group (with Prof. Dale Gary), which operates the Expanded Owens Valley Solar Array (EOVSA). He is currently leading a NSF-funded project to upgrade EOVSA to EOVSA-15, which will expand it to a 15-antenna array and enable broadband imaging spectropolarimetry for the array.
He was the recipient of AAS Solar Physics Division’s Karen Harvey Prize in 2023, the National Science Foundation’s CAREER Award in 2017, and the NASA/UCAR Jack Eddy Fellowship in 2013. He served as a Committee Member of the Solar Physics Division of the American Astronomical Society (2019–2021). He has recently served on the Solar & Heliophere Panel of the NASEM 2024-2033 Solar & Space Physics Decadal Survey. At NJIT, he serves as the Director of the Applied Physics Graduate Program (2020–present). His research is funded by multiple grants from NSF and NASA, totaling several million US dollars as PI.
Inquiries on potential Ph.D. or postdoctoral positions are always welcome. Please contact him by email.
Download his Curriculum Vitae.
PhD in Astronomy, 2013
University of Virginia
MS in Astrophysics, 2008
University of Chinese Academy of Sciences
BS in Physics, 2005
Peking University
Large eruptions on the Sun and main drivers of Space Weather
Develop and commission new instrumentation for solar astronomy
The fundamental process for releasing magnetic energy
Mechanisms for accelerating particles to high energies
Shocks and Waves on the Sun
Origin of intense radio bursts that affect GPS reception
A series of studies using data from the Karl G. Jansky Very Large Array have revealed a special type of shocks, called “termination shocks”, as an outstanding candidate for particle acceleration in the core solar flare region.
Our new study published in Nature Astronomy reports unprecedented measurements of the magnetic field and relativistic of a large-scale magnetic reconnection current sheet – the “central engine” that powers the mega solar flare on 2017 September 10. Click links below for featured stories by funding agencies, institutions, and media outlets.
Check this SAO/NASA ADS Library for comprehensive list