activity
20072025
most citedStreamer Waves Driven by Coronal Mass Ejections

78 citations · 178 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

Towards DM-free search for Fast Radio Bursts with Machine Learning -- I. An implementation on multibeam data

Yao Chen, Rui Luo, Chen Wang +13

Searching for fleeting radio transients like fast radio bursts (FRBs) with wide-field radio telescopes has become a common challenge in data-intensive science. Conventional algorit…

astro-ph.SR2025

Solar jet-induced perturbation propagating through coronal loops and in-loop electron beam transport indicated by type II and type N radio bursts

Yingli Cui, Xiangliang Kong, Zhentong Li +12

Solar type II radio bursts are commonly attributed to coronal shocks driven by coronal mass ejections (CMEs). However, some metric type II bursts have occasionally been reported to…

astro-ph.SR2025

A Wide-band High-frequency Type-II Solar Radio Burst

V. Vasanth, Yao Chen, G. Michalek

Type-II radio bursts are typically observed below ~ 400 MHz, with narrow-band slowly-drifting fundamental and harmonic structures. Here we report an unusual high-frequency wide-ban…

astro-ph.SR2010★ 78 cited

Streamer Waves Driven by Coronal Mass Ejections

Y. Chen, H. Q. Song, B. Li +4

Between July 5th and July 7th 2004, two intriguing fast coronal mass ejection(CME)-streamer interaction events were recorded by the Large Angle and Spectrometric Coronagraph (LASCO…

astro-ph.SR2009★ 53 cited

Intrinsic Instability of Coronal Streamers

Y. Chen, X. Li, H. Q. Song +3

Plasma blobs are observed to be weak density enhancements as radially stretched structures emerging from the cusps of quiescent coronal streamers. In this paper, it is suggested th…

astro-ph2007★ 47 cited

Catastrophic eruption of magnetic flux rope in the corona and solar wind with and without magnetic reconnection

Y. Chen, Y. Q. Hu, S. J. Sun

It is generally believed that the magnetic free energy accumulated in the corona serves as a main energy source for solar explosions such as coronal mass ejections (CMEs). In the f…