37 citations · 391 across the 33 of their papers we have counts for
33 papers
Responses of a Coronal Hole to a Fast Flare-Driven Coronal Wave
Xiaofan Zhang, Huadong Chen, Guiping Zhou +12
Coronal waves, significant solar phenomena, act as diagnostic tools for scientists studying solar atmosphere properties. Here, we present a novel observation detailing how a corona…
A Flare-related Decimetric Type-IV Radio Burst Induced by the X2 Radiation of Electron Cyclotron Maser Emission
Maoshui Lv, Ze Zhong, Xiangliang Kong +9
The radiation mechanism of decimetric wideband and pulsating radio bursts from the Sun (in terms of decimetric type-IV (t-IVdm) burst) and other flaring stars is a long-standing pr…
The magnetic origin of the mystery of rare H Moreton waves
Ze Zhong, Yao Chen, Y. W. Ni +4
Over the past three decades, a lot of coronal fast-mode waves were detected by space missions, but their counterparts in the chromosphere, called the Moreton waves, were rarely cap…
Filament eruption by multiple reconnections
Y. Liu, G. P. Ruan, B. Schmieder +5
Filament eruption is a common phenomenon in solar activity, but the triggering mechanism is not well understood. We focus our study on a filament eruption located in a complex nest…
A Multi-Peak Solar Flare with a High Turnover Frequency of The Gyrosynchrotron Spectra from the Loop-Top Source
Zhao Wu, Alexey Kuznetsov, Sergey Anfinogentov +8
The origin of multiple peaks in lightcurves of various wavelengths remains illusive during flares. Here we discuss the flare of SOL2023-05-09T03:54M6.5 with six flux peaks as recor…
A Type II Radio Burst Driven by a Blowout Jet on the Sun
Zhenyong Hou, Hui Tian, Wei Su +5
Type II radio bursts are often associated with coronal shocks that are typically driven by coronal mass ejections (CMEs) from the Sun. Here, we conduct a case study of a type II ra…
An extreme ultraviolet wave associated with the possible expansion of sheared arcades
Yihan Liu, Ruisheng Zheng, Liang Zhang +4
Context. Solar extreme ultraviolet (EUV) waves are propagating disturbances in the corona, and they usually accompany with various solar eruptions, from large-scale coronal mass ej…
Why "solar tsunamis" rarely leave their imprints in the chromosphere
Ruisheng Zheng, Yihan Liu, Wenlong Liu +10
Solar coronal waves frequently appear as bright disturbances that propagate globally from the eruption center in the solar atmosphere, just like the tsunamis in the ocean on Earth.…
Imaging Preflare Broadband Pulsations in the Decimetric-metric Wavelengths
Maoshui Lv, Baolin Tan, Ruisheng Zheng +4
Preflare activities contain critical information about the pre-cursors and causes of solar eruptions. Here we investigate the characteristics and origin of a group of broadband pul…
Composition Comparison between ICMEs from Active Regions and Quiet-Sun Regions
Jinrong Li, Hongqiang Song, Qi Lv +4
The composition, including the ionic charge states and elemental abundances of heavy elements, within interplanetary coronal mass ejections (ICMEs) has tight correlations with thei…
The deformation of an erupting magnetic flux rope in a confined solar flare
Ruisheng Zheng, Yihan Liu, Liang Zhang +7
Magnetic flux ropes (MFRs), sets of coherently twisted magnetic field lines, are believed as core structures of various solar eruptions. Their evolution plays an important role to…
On the Nature of the Three-part Structure of Solar Coronal Mass Ejections
Hongqiang Song, Jie Zhang, Leping Li +4
Coronal mass ejections (CMEs) result from eruptions of magnetic flux ropes (MFRs) and can possess a three-part structure in white-light coronagraphs, including a bright front, dark…
Birth places of extreme ultraviolet waves driven by impingement of solar jets upon coronal loops
Liang Zhang, Ruisheng Zheng, Huadong Chen +1
Solar extreme ultraviolet (EUV) waves are large-scale propagating disturbances in the corona. It is generally believed that the vital key for the formation of EUV waves is the rapi…
Twin extreme ultraviolet waves in the solar corona
Ruisheng Zheng, Bing Wang, Liang Zhang +2
Solar extreme ultraviolet (EUV) waves are spectacular propagating disturbances with EUV enhancements in annular shapes in the solar corona. These EUV waves carry critical informati…
Three-dimensional Propagation of the Global EUV Wave associated with a solar eruption on 2021 October 28
Zhenyong Hou, Hui Tian, Jing-Song Wang +16
We present a case study for the global extreme ultraviolet (EUV) wave and its chromospheric counterpart `Moreton-Ramsey wave' associated with the second X-class flare in Solar Cycl…
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions
Ruisheng Zheng, Liang Zhang, Changhui Rao +4
It is generally believed that filament formation involves a process of the accumulation of magnetic energy. However, in this paper we discuss the idea that filaments will not erupt…
Compound eruptions of twin flux ropes in a solar active region
Ruisheng Zheng, Liang Zhang, Bing Wang +6
Compound eruptions represent that multiple closely spaced magnetic structures erupt consecutively within a short interval, and then lead to a single flare and a single CME. However…
The Inhomogeneity of Composition along the Magnetic Cloud Axis
Hongqiang Song, Qiang Hu, Xin Cheng +6
It is generally accepted that CMEs result from eruptions of magnetic flux ropes, which are dubbed as magnetic clouds in interplanetary space. The composition (including the ionic c…
Solar Cycle Dependence of ICME Composition
Hongqiang Song, Leping Li, Yanyan Sun +3
Coronal mass ejections (CMEs) are one of the most energetic explosions in the solar atmosphere, and their occurrence rates exhibit obvious solar cycle dependence with more events t…
Do All Interplanetary Coronal Mass Ejections Have A Magnetic Flux Rope Structure Near 1 AU?
Hongqiang Song, Jie Zhang, Xin Cheng +6
Interplanetary coronal mass ejections (ICMEs) often consist of a shock wave, sheath region, and ejecta region. The ejecta regions are divided into two broad classes: magnetic cloud…
Formation of a tiny flux rope in the center of an active region driven by magnetic flux emergence, convergence, and cancellation
Ruisheng Zheng, Yao Chen, Bing Wang +2
Flux ropes are generally believed to be core structures of solar eruptions that are significant for the space weather, but their formation mechanism remains intensely debated. We r…
The initiation of a solar streamer blowout coronal mass ejection arising from the streamer flank
Ruisheng Zheng, Yao Chen, Bing Wang
Streamer blowout (SBO) coronal mass ejections (CMEs) represent a particular class of CMEs that are characterized by a gradual swelling of the overlying streamer and a slow CME cont…
An Extreme Ultraviolet Wave Associated with A Solar Filament Activation
Ruisheng Zheng, Yao Chen, Bing Wang +1
Extreme ultraviolet (EUV) waves are impressive coronal propagating disturbances. They are closely associated with various eruptions, and can used for the global coronal seismology…
The Structure of Solar Coronal Mass Ejections in the Extreme-Ultraviolet Passbands
H. Q. Song, J. Zhang, L. P. Li +5
So far most studies on the structure of coronal mass ejections (CMEs) are conducted through white-light coronagraphs, which demonstrate about one third of CMEs exhibit the typical…