Solar Radio Bursts
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 flares are sudden energy release events in the solar corona, resulting from magnetic reconnection, that accelerate particles and …
Rohit Sharma,
Marina Battaglia,
Yingjie Luo,
Bin Chen,
Sijie Yu
Drifting pulsation structures (DPSs) are important radio fine structures usually observed at the beginning of eruptive solar flares. It …
Marian Karlický,
Bin Chen,
Dale E. Gary,
Jana Kašparová,
Jan Rybák
Magnetic reconnection, the central engine that powers explosive phenomena throughout the universe, is also perceived to be one of the …
Bin Chen,
Sijie Yu,
Marina Battaglia,
Samaiyah Farid,
Antonia Savcheva,
Katharine K. Reeves,
Säm Krucker,
T.~S. Bastian,
Fan Guo,
Svetlin Tassev
Fiber bursts are a type of fine structure that is often superposed on type IV radio continuum emission during solar flares. Although …
Zhitao Wang,
Bin Chen,
Dale E. Gary
We report observations of type III radio bursts at decimeter wavelengths (type IIIdm bursts)—signatures of suprathermal electron beams …
Bin Chen,
T. Bastian,
S. White,
D. Gary,
R. Perley,
M. Rupen,
B. Carlson
We present the first interferometric observation of a zebra-pattern radio burst with simultaneous high spectral (ensuremath≈1 MHz) and …
Bin Chen,
T. Bastian,
D. Gary,
Ju Jing
In this paper, we devote ourselves to interpreting the short-lived absorptive type III-like microwave bursts in the 2006 December 13 …
Bin Chen,
Yihua Yan
Through the data around 3 GHz from the Radio Spectrometer in Huairou, Beijing, zebra-pattern structures from the 21 April 2002 event …
Bin Chen,
Yihua Yan
On 2006 December 13 during the solar minimum, the superactive region NOAA 10930 at the S05W33 disk location produced an X3.4/4B flare …
Yihua Yan,
Jing Huang,
Bin Chen,
Takashi Sakurai