64 citations · 407 across the 15 of their papers we have counts for
15 papers
Source Imaging of a Moving Type-IV Solar Radio Burst and its Role in Tracking Coronal Mass Ejection From the Inner to the Outer Corona
V. Vasanth, Yao Chen, Maoshui Lv +5
Source imaging of solar radio bursts can be used to track energetic electrons and associated magnetic structures. Here we present a combined analysis of data at different wavelengt…
Formation of Large Scale Coronal Loops Interconnecting Two Active Regions Through Gradual Magnetic Reconnection and Associated Heating Process
Guohui Du, Yao Chen, Chunming Zhu +5
Coronal loops interconnecting two active regions, called as interconnecting loops (ILs), are prominent large-scale structures in the solar atmosphere. They carry a significant amou…
Two-stage energy release process of a confined flare with double HXR peaks
Hao Ning, Yao Chen, Zhao Wu +5
A complete understanding of the onset and subsequent evolution of confined flares has not been achieved. Earlier studies mainly analyzed disk events so as to reveal their magnetic…
Double Coronal X-ray and Microwave Sources Associated With A Magnetic Breakout Solar Eruption
Yao Chen, Zhao Wu, Wei Liu +4
Double coronal hard X-ray (HXR) sources are believed to be critical observational evidence of bi-directional energy release through magnetic reconnection in a large-scale current s…
EUV and Magnetic Activities Associated with Type-I Solar Radio Bursts
Chuanyang Li, Yao Chen, Bing Wang +4
Type-I bursts (i.e. noise storms) are the earliest-known type of solar radio emission at the metre wavelength. They are believed to be excited by non-thermal energetic electrons ac…
Interaction of two filaments in a long filament channel associated with twin coronal mass ejections
Ruisheng Zheng, Qingmin Zhang, Yao Chen +4
Using the high-quality observations of the Solar Dynamics Observatory, we present the interaction of two filaments (F1 and F2) in a long filament channel associated with twin coron…