activity
20102026
most citedObservation and Simulation of Longitudinal Oscillations of an Active Region Prominence

99 citations · 1k across the 57 of their papers we have counts for

collaborators

59 papers

astro-ph.SR2026

Observations of a Solar Jet Triggered by Reconnection between Super-penumbral Fibrils and a Mini-filament

Liheng Yang, Xiaoli Yan, Qingmin Zhang +10

Coronal jets are highly dynamic phenomena in the solar atmosphere, yet their driving mechanisms remain an active topic of investigation. In this paper, we report a coronal jet trig…

astro-ph.SR2026

Three-dimensional evolution of a solar filament with multipoint observations

Qingmin Zhang, Jun Dai, Beili Ying +6

In this paper, we first devise a geometrical model, featuring a torus-like flux rope based on the shape of 3DCORE model. The global shape of the torus is an ellipse, while the cros…

astro-ph.SR2026

Characterizing the 3D evolution of two successive CMEs heading for Mercury

Yanjie Zhang, Qingmin Zhang, Huadong Chen +3

We studied two successive coronal mass ejections (CMEs) that erupted from the same active region (AR 12994) on 2022 April 15 and propagated toward Mercury. Using multi-view observa…

astro-ph.SR2026

Herringbone structures during an X-class eruptive flare

Qingmin Zhang, Zongjun Ning, Xingyao Chen +3

In this paper, we report quasi-periodic herringbone structures during the impulsive phase of an X-class flare, coinciding with the distinct acceleration phase of eruptive prominenc…

astro-ph.SR2025

Extreme Ultraviolet Wave and Quasi-periodic Pulsations during an eruptive M-class Flare

Shuyue Li, Qingmin Zhang, Haisheng Ji +3

In this paper, we report multiwavelength and multipoint observations of the prominence eruption originating from active region 11163, which generated an M3.5 class flare and a coro…

astro-ph.SR2025

Tracking an eruptive intermediate prominence originating from the farside of the Sun

Qingmin Zhang, Wenwei Pan, Beili Ying +7

In this paper, we carry out multiwavelength and multiview observations of the eruption of an intermediate prominence originating from the farside of the Sun on 2023 March 12. The s…

astro-ph.SR2025

Transverse Oscillations of Coronal Loops Induced by a Jet-Related Confined Flare on 11 July 2022

Musheng Lin, Ya Wang, Liheng Yang +4

In this article, we report the multiwavelength and multiview observations of transverse oscillations of two loop strands induced by a jet-related, confined flare in active region N…

astro-ph.SR2024

Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops

Leping Li, Hongqiang Song, Yijun Hou +11

Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…

astro-ph.SR2024

Sympathetic solar eruption on 2024 February 9

Shu-Yue Li, Qing-Min Zhang, Bei-Li Ying +3

In this paper, we perform a follow-up investigation of the solar eruption originating from active region (AR) 13575 on 2024 February 9. The primary eruption of a hot channel (HC) g…

astro-ph.SR2024

Tracking an eruptive prominence using multiwavelength and multiview observations on 2023 March 7

Qingmin Zhang, Yudi Ou, Zhenghua Huang +2

In this paper, we carry out multiwavelength and multiview observations of the prominence eruption, which generates a C2.3 class flare and a coronal mass ejection (CME) on 2023 Marc…

astro-ph.SR2024

Asymmetric Hard X-ray Radiation of Two Ribbons in a Thermal-Dominated C-Class Flare

Guanglu Shi, Li Feng, Jun Chen +9

The asymmetry in hard X-ray (HXR) emission at the footpoints (FPs) of flare loops is a ubiquitous feature closely associated with nonthermal electron transport. We analyze the asym…

astro-ph.SR2024

Association between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence

Jianchao Xue, Li Feng, Hui Li +31

Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here we present two failed prominence eru…

astro-ph.SR2024

Observation of a large-scale filament eruption initiated by two small-scale erupting filaments pushing out from below

Yongliang Song, Jiangtao Su, Qingmin Zhang +9

Filament eruptions often result in flares and coronal mass ejections (CMEs). Most studies attribute the filament eruptions to their instabilities or magnetic reconnection. In this…

astro-ph.SR2024

Spectral and Imaging Observations of a C2.3 White-Light Flare from the Advanced Space-Based Solar Observatory (ASO-S) and the Chinese H Solar Explorer (CHASE)

Qiao Li, Ying Li, Yang Su +27

Solar white-light flares are characterized by an enhancement in the optical continuum, which are usually large flares (say X- and M-class flares). Here we report a small C2.3 white…

astro-ph.SR2024

Circular-ribbon flares and the related activities

Qingmin Zhang

In this paper, I will present the recent progress on circular-ribbon flares (CRFs) and their related activities, including coronal jets, filaments, CMEs, radio bursts, coronal dimm…

astro-ph.SR2024

Transverse oscillation of prominence and filament induced by an EUV wave from the farside of the Sun

Yanjie Zhang, Qingmin Zhang, De-chao Song +1

In this paper, we report our multi-angle observations of the transverse oscillation of a prominence and a filament induced by an EUV wave originating from the farside of the Sun on…

astro-ph.SR2024

A Statistical Study of Solar White-Light Flares Observed by the White-light Solar Telescope of the Lyman-alpha Solar Telescope on the Advanced Space-based Solar Observatory (ASO-S/LST/WST) at 360 nm

Zhichen Jing, Ying Li, Li Feng +26

Solar white-light flares (WLFs) are those accompanied by brightenings in the optical continuum or integrated light. The White-light Solar Telescope (WST), as an instrument of the L…

astro-ph.SR2024

Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event

Liheng Yang, Xiaoli Yan, Zhike Xue +5

Previous studies have revealed that solar coronal jets triggered by the eruption of mini-filaments (MFs) conform to the famous magnetic-breakout mechanism. In such scenario, a brea…

astro-ph.SR2023

Simultaneous Horizontal and Vertical Oscillation of a Quiescent Filament observed by CHASE and SDO

Jun Dai, Qingmin Zhang, Ye Qiu +5

In this paper, we present the imaging and spectroscopic observations of the simultaneous horizontal and vertical large-amplitude oscillation of a quiescent filament triggered by an…

astro-ph.SR2023

Energetics of a solar flare and a coronal mass ejection generated by a hot channel eruption

Qingmin Zhang, Weilin Teng, Dong Li +2

Hot channels (HCs) are prevalent in the solar corona and play a critical role in driving flares and CMEs. In this paper, we estimate the energy contents of an X1.4 eruptive flare w…

astro-ph.SR2023

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…

astro-ph.SR2023★ 5 cited

Transverse vertical oscillations during the contraction and expansion of coronal loops

Qingmin Zhang, Yuhao Zhou, Chuan Li +5

In this paper, we carry out a detailed analysis of the M1.6 class eruptive flare occurring in NOAA active region 13078 on 2022 August 19. The flare is associated with a fast corona…

astro-ph.SR2023★ 6 cited

Global energetics of solar powerful events on 6 September 2017

Dong Li, Alexander Warmuth, Jincheng Wang +9

Solar flares and coronal mass ejections (CMEs) are thought to be the most powerful events on the Sun. They can release energy as high as 10^32 erg in tens of minutes,and could prod…

astro-ph.SR2023★ 6 cited

High-resolution He I 10830 Å narrowband imaging for precursors of chromospheric jets and their quasi-periodic properties

Ya Wang, Qingmin Zhang, Zhenxiang Hong +3

Solar jets are well-collimated plasma ejections in the solar atmosphere. They are prevalent in active regions, the quiet Sun, and even coronal holes. They display a range of temper…