254 citations · 2.2k across the 35 of their papers we have counts for
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Data-constrained Magnetohydrodynamic Simulation of an Intermediate Solar Filament Eruption
Yang Guo, Jinhan Guo, Yiwei Ni +5
Solar eruptive activities could occur in weak magnetic field environments and over large spatial scales, especially relevant to eruptions involving intermediate or quiescent solar…
Thermodynamic and Magnetic Topology Evolution of the X1.0 Flare on 2021 October 28 Simulated by a Data-driven Radiative Magnetohydrodynamic Model
Jin-han Guo, Yi-wei Ni, Ze Zhong +6
Solar filament eruptions, flares and coronal mass ejections (CMEs) are manifestations of drastic release of energy in the magnetic field, which are related to many eruptive phenome…
Formation of Quiescent Prominence Magnetic Field by Supergranulations
Qingjun Liu, Chun Xia
To understand the formation of quiescent solar prominences, the origin of their magnetic field structures, i.e., magnetic flux ropes (MFRs), must be revealed. We use three-dimensio…
A formation mechanism for the large plumes in the prominence
Jincheng Wang, Xiaoli Yan, Zhike Xue +5
To understand the formation mechanism of large plumes in solar prominences, we investigate the formation process of two such phenomena. We studied the dynamic and thermal propertie…
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…
Measuring three-dimensional shapes of stable solar prominences using stereoscopic observations from SDO and STEREO
Chengrui Zhou, Chun Xia, Yuandeng Shen
Although the real shapes and trajectories of erupting solar prominences in three dimensions have been intensively studied, the three-dimensional (3D) shapes of stable prominences b…