activity
20032022
most citedFirst Evidence of Coexisting EIT Wave and Coronal Moreton Wave from SDO/AIA Observations

119 citations · 701 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2022★ 14 cited

Cross-loop propagation of a quasi-periodic extreme-ultraviolet wave train triggered by successive stretching of magnetic field structures during a solar eruption

Zheng Sun, Hui Tian, P. F. Chen +4

Solar extreme-ultraviolet (EUV) waves generally refer to large-scale disturbances propagating outward from sites of solar eruptions in EUV imaging observations. Using the recent ob…

astro-ph.SR2022★ 22 cited

Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes

J. H. Guo, Y. W. Ni, Y. H. Zhou +3

Many prominences are supported by magnetic flux ropes. One important question is how we can determine whether the flux rope is weakly-twisted or strongly-twisted. In this paper, we…

astro-ph.SR2022

Dynamics and Kinematics of the EUV Wave Event on 6 May 2019

Ramesh Chandra, P. F. Chen, Pooja Devi +2

We present here the kinematics of the EUV wave associated with a GOES M1.0-class solar flare, which originates in NOAA AR 12740. The event is thoroughly observed with Atmospheric I…

astro-ph.SR2022★ 13 cited

Quantifying the Magnetic Structure of a Coronal Shock Producing a Type II Radio Burst

W. Su, T. M. Li, X. Cheng +9

Type II radio bursts are thought to be produced by shock waves in the solar atmosphere. However, what magnetic conditions are needed for the generation of type II radio bursts is s…

astro-ph.SR2021★ 28 cited

Magnetic Twists of Solar Filaments

Jinhan Guo, Yiwei Ni, Ye Qiu +3

Solar filaments are cold and dense materials situated in magnetic dips, which show distinct radiation characteristics compared to the surrounding coronal plasma. They are associate…

astro-ph.SR2021

Data-constrained Magnetohydrodynamic Simulation of a Long Duration Eruptive Flare

Yang Guo, Ze Zhong, M. D. Ding +3

We perform a zero- magnetohydrodynamic simulation for the C7.7 class flare initiated at 01:18 UT on 2011 June 21 using the Message Passing Interface Adaptive Mesh Refinement Ver…