Dr. Bin Chen is a Professor of Physics at the New Jersey Institute of Technology. He studies solar flares and coronal mass ejections—the solar system’s largest explosions and major drivers of space weather—using radio and multi-wavelength observations to understand their underlying physical processes. He also develops radio instrumentation for solar and space weather research.

He is Principal Investigator of the Owens Valley Solar Arrays (OVSA), an NSF-funded community facility comprising the Expanded Owens Valley Solar Array (EOVSA) and the solar and space weather programs of the Owens Valley Radio Observatory’s Long Wavelength Array (OVRO-LWA). He leads the NSF-funded EOVSA-15 upgrade, which will expand EOVSA to 15 antennas and enable broadband imaging spectropolarimetry.

His honors include the AAS Solar Physics Division’s Karen Harvey Prize (2023), the NSF CAREER Award (2017), and the NASA/UCAR Jack Eddy Fellowship (2013). He is the Vice Chair of the AAS Solar Physics Division (August 2026–present) and previously served on its committee (2019–2021). He also served on the Sun and Heliosphere Panel of the 2024–2033 Solar and Space Physics Decadal Survey and directed NJIT’s Applied Physics Graduate Program from 2020 to 2026. He has secured several million dollars in NSF and NASA research funding as PI.

Inquiries about Ph.D. and postdoctoral opportunities are welcome by email.

Download his Curriculum Vitae.

Interests
  • Solar Flares
  • Corona Mass Ejections
  • Space Weather
  • Magnetic Reconnection
  • Particle Acceleration
  • Radio Astronomy and instrumentation
Education
  • PhD in Astronomy, 2013

    University of Virginia

  • MS in Astrophysics, 2008

    University of Chinese Academy of Sciences

  • BS in Physics, 2005

    Peking University

Meet the Team

Faculty

Avatar

Prof. Bin Chen

Professor of Physics
OVSA PI

Avatar

Prof. Sijie Yu

Assistant Professor of Physics
EOVSA Project Scientist

Research Faculty & Staff

Avatar

Dr. Gregory Fleishman

Distinguished Research Professor

Avatar

Dr. Gelu Nita

Research Professor

Avatar

Dr. Owen Giersch

EOVSA Chief Observer

Avatar

Dr. Caius Selhorst

EOVSA Observer & Data Manager

Avatar

Dr. Peijin Zhang

OVRO-LWA Solar Project Scientist

Postdoctoral Fellows

Avatar

Dr. Yuqian Wei

Postdoctoral Fellow; PhD, 2023

Avatar

Dr. Meiqi Wang

Postdoctoral Fellow; PhD, 2025

Graduate Students

Avatar

Ivan Oparin

Ph.D. Candidate (Advisor - Chen/Fleishman)

Avatar

Stasia Kuske

Ph.D. Candidate (Advisor - Chen/Nita)

Avatar

Anshika Singh

Graduate Student (Advisor - Chen)

Avatar

Mallory Wickline

Graduate Student (Advisor - Yu/Chen)

Avatar

Louis Seyfritz

Graduate Student (Advisor - Chen)

Alumni

Avatar

Dr. Surajit Mondal

Postdoctoral Fellow, 2021-2025; Now scientist at NCRA, India

Avatar

Dr. Xingyao Chen

Postdoctoral Fellow, 2023-2025; Now scientist at NSSC, CAS

Avatar

Dr. Yingjie Luo

PhD, 2022; Now postdoc fellow at Univ. of Glasgow

Avatar

Sabastian Fernandes

UG Research Assistant (2022-2026)

Avatar

Dr. Zhitao Wang

PhD, 2017; Now Big Data Engineer at HSBC

Avatar

Samantha Lomuscio

UG Research Assistant (2017-2020); Now Algorithm Developer at JHU/APL

Avatar

Sylwia Janiak

UG Research Assistant (2016-2019)

Avatar

Lindsey Gray

UG Research Assistant (summer 2016); Now graduate student at Wake Forest Univ.

New study published in Nature Astronomy
We have a new study published in Nature Astronomy. The study, led by Dr. Sijie Yu of our group, presents aurora-like radio bursts above a Sunspot with the Karl G. Jansky Very Large Array. The results may have profound implications on the interpretation of similar bursts observed on other stars. See press release story at this link.
New study published in Nature Astronomy

Research Projects

*
Coronal Mass Ejections

Coronal Mass Ejections

Large eruptions on the Sun and main drivers of Space Weather

Instrumentation

Instrumentation

Develop and commission new instrumentation for solar astronomy

Magnetic Reconnection

Magnetic Reconnection

The fundamental process for releasing magnetic energy

Particle Acceleration

Particle Acceleration

Mechanisms for accelerating particles to high energies

Shocks and Waves

Shocks and Waves

Shocks and Waves on the Sun

Solar Radio Bursts

Solar Radio Bursts

Origin of intense radio bursts that affect GPS reception

Publication List

Check this SAO/NASA ADS Library for comprehensive list

Quickly discover relevant content by filtering publications.
(2024). Energetic Electrons Accelerated and Trapped in a Magnetic Bottle above a Solar Flare Arcade. The Astrophysical Journal.

Cite DOI ADS

(2024). Study of Particle Acceleration Using Fine Structures and Oscillations in Microwaves from the Electron Cyclotron Maser. The Astrophysical Journal.

PDF Cite DOI

(2024). Episodic Energy Release during the Main and Post-impulsive Phases of a Solar Flare. The Astrophysical Journal.

PDF Cite DOI

(2024). Doppler signature of a possible termination shock in an off-limb solar flare. Monthly Notices of the Royal Astronomical Society.

PDF Cite DOI

(2024). Detection of long-lasting aurora-like radio emission above a sunspot. Nature Astronomy.

Cite DOI ADS

(2023). The Solar Origin of an In Situ Type III Radio Burst Event. The Astrophysical Journal.

PDF Cite DOI

(2023). Fine Structures of Radio Bursts from Flare Star AD Leo with FAST Observations. The Astrophysical Journal.

PDF Cite DOI

(2023). Defining the Middle Corona. Solar Physics.

PDF Cite DOI

(2023). Multifrequency Microwave Imaging of Weak Transients from the Quiet Solar Corona. The Astrophysical Journal.

PDF Cite DOI

(2023). Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions. Frontiers in Astronomy and Space Sciences.

PDF Cite DOI

(2022). Microwave Imaging of Quasi-Periodic Pulsations at Flare Current Sheet. Nature Communications.

Cite DOI

(2022). Multiple Regions of Nonthermal Quasiperiodic Pulsations during the Impulsive Phase of a Solar Flare. The Astrophysical Journal.

Cite DOI

(2022). A Model of Double Coronal Hard X-Ray Sources in Solar Flares. The Astrophysical Journal.

Cite DOI

(2022). Implications for Additional Plasma Heating Driving the Extreme-ultraviolet Late Phase of a Solar Flare with Microwave Imaging Spectroscopy. The Astrophysical Journal.

Cite DOI

(2022). Modeling Electron Acceleration and Transport in the Early Impulsive Phase of the 2017 September 10th Solar Flare. The Astrophysical Journal.

Cite DOI

(2022). Solar Flare Accelerates Nearly All Electrons in a Large Coronal Volume. Nature.

Cite DOI ADS

(2022). The Origin of Underdense Plasma Downflows Associated with Magnetic Reconnection in Solar Flares. Nature Astronomy.

Cite DOI

(2021). Coronal Magnetic Field Measurements along a Partially Erupting Filament in a Solar Flare. The Astrophysical Journal.

Cite DOI

(2021). Multiple Electron Acceleration Instances during a Series of Solar Microflares Observed Simultaneously at X-Rays and Microwaves. The Astrophysical Journal.

Cite DOI

Contact