65 citations · 523 across the 40 of their papers we have counts for
11 papers · 1 filter
Simultaneous detection of flare-associated kink oscillations and extreme-ultraviolet waves
Dong Li, Zhenyong Hou, Xianyong Bai +5
Kink oscillations, which are frequently observed in coronal loops and prominences, are often accompanied by extreme-ultraviolet (EUV) waves. However, much more needs to be explored…
The triggering process of an X-class solar flare on a small quadrupolar active region
Qiao Song, Jing-Song Wang, Xiaoxin Zhang +13
The occurrence of X-class solar flares and their potential impact on the space weather often receive great attention than other flares. But predicting when and where an X-class fla…
Internal activities in a solar filament and heating to its threads
Hengyuan Wei, Zhenghua Huang, Chuan Li +5
Filaments are one of the most common features in the solar atmosphere, and are of significance in solar, stellar and laboratory plasma physics. Using data from the Chinese H Sol…
Observation of two splitting processes in a partial filament eruption on the sun: the role of breakout reconnection
Zheng Sun, Ting Li, Hui Tian +5
Partial filament eruptions have often been observed, however, the physical mechanisms that lead to filament splitting are not yet fully understood. In this study, we present a uniq…
A revised graduated cylindrical shell model and its application to a prominence eruption
Qing-Min Zhang, Zhen-Yong Hou, Xian-Yong Bai
In this paper, the well-known graduated cylindrical shell (GCS) model is slightly revised by introducing longitudinal and latitudinal deflections of prominences originating from ac…
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…
Traveling kink oscillations of coronal loops launched by a solar flare
Dong Li, Xianyong Bai, Hui Tian +5
We investigate the traveling kink oscillation triggered by a solar flare on 2022 September 29. The observational data is mainly measured by the Solar Upper Transition Region Imager…
Full velocities and propagation directions of coronal mass ejections inferred from simultaneous full-disk imaging and Sun-as-a-star spectroscopic observations
Hong-peng Lu, Hui Tian, He-chao Chen +6
Coronal mass ejections (CMEs) are violent ejections of magnetized plasma from the Sun, which can trigger geomagnetic storms, endanger satellite operations and destroy electrical in…
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.…
Heating of quiescent coronal loops caused by nearby eruptions observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager
Leping Li, Hui Tian, Huadong Chen +5
How structures, e.g., magnetic loops, in the upper atmosphere, i.e., the transition region and corona, are heated and sustained is one of the major unresolved issues in solar and s…
The Solar Upper Transition Region Imager (SUTRI) onboard the SATech-01 satellite
Xianyong Bai, Hui Tian, Yuanyong Deng +56
The Solar Upper Transition Region Imager (SUTRI) onboard the Space Advanced Technology demonstration satellite (SATech-01), which was launched to a sun-synchronous orbit at a heigh…