60 citations · 536 across the 28 of their papers we have counts for
28 papers
Repeated Sunspot Light Bridge Jets Associated with Slipping Base Brightenings
Yadan Duan, Xiaoli Yan, Yuhang Gao +3
Light bridge (LB) jets offer a unique window into small-scale eruptive phenomena within sunspots, the Sun's strongest magnetic environments; however, their generation mechanism rem…
Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge
Tianyuan Chen, Xiaoli Yan, Zhike Xue +9
We used high-resolution observations from the New Vacuum Solar Telescope and the Solar Dynamics Observatory to carry out a detailed multiwavelength analysis of the fine structures…
Fine Structure and Formation Mechanism of a Sunspot Bipolar Light Bridge in NOAA AR 13663
Fangfang Qiao, Hao Li, Jiasheng Wang +3
Bipolar Light Bridges (BLBs) are bright regions located between sunspot umbrae of opposite magnetic polarity. They are typically characterized by strong magnetic fields and intense…
Resolving Interchange Reconnection Dynamics in a Fan-Spine-like Topology Observed by Solar Orbiter
Yadan Duan, Xiaoli Yan, Junchao Hong +5
Interchange reconnection is believed to play a significant role in the production of solar jets and solar wind. However, the dynamics of interchange reconnection in the low corona…
Reconnection nanojets in an erupting solar filament with unprecedented high speeds
Yuhang Gao, Hui Tian, David Berghmans +4
Solar nanojets are small-scale jets generated by component magnetic reconnection, characterized by collimated plasma motion perpendicular to the reconnecting magnetic field lines.…
Ubiquitous Small-scale EUV Upflow-Like Events above Network Regions Observed by the Solar Orbiter/Extreme Ultraviolet Imager
Yadan Duan, Hechao Chen, Zhenyong Hou +2
Universal small-scale solar activity in quiet region are suggested to be a potential source of solar wind and the upper solar atmosphere. Here, with the high-resoltion 174 Å~imagin…
Fast Downflows Observed during a Polar Crown Filament Eruption
Zheng Sun, Hui Tian, Ting Li +2
Solar filaments can undergo eruptions and result in the formation of coronal mass ejections (CMEs), which could significantly impact planetary space environments. Observations of e…
On the Determining Physical Factor of Jet-Related Coronal Mass Ejection's Morphology in the High Corona
Yadan Duan, Yuandeng Shen, Zehao Tang +2
A solar jet can often cause coronal mass ejections (CMEs) with different morphologies in the high corona, for example, jet-like CMEs, bubble-like CMEs, and so-called twin CMEs that…
Formation of Fan-spine Magnetic Topology through Flux Emergence and Subsequent Jet Production
Yadan Duan, Hui Tian, Hechao Chen +4
Fan-spine magnetic structure, as a fundamental three-dimensional topology in magnetic reconnection theory, plays a crucial role in producing solar jets. However, how fan-spine conf…
Double-decker Pair of Flux Ropes Formed by Two Successive Tether-cutting Eruptions
Yuandeng Shen, Dongxu Liu, Surui Yao +7
Double-decker filaments and their eruptions have been widely observed in recent years, but their physical formation mechanism is still unclear. Using high spatiotemporal resolution…
Stereoscopic Observation of Simultaneous Longitudinal and Transverse Oscillations in a Single Filament Driven by Two-sided-loop Jet
Song Tan, Yuandeng Shen, Xinping Zhou +4
We report the first observations of simultaneous large-amplitude longitudinal and transverse oscillations of a quiescent filament trigged by a two-sided-loop jet formed by the magn…
Macrospicules and Their Connection to Magnetic Reconnection in the Lower Atmosphere
Yadan Duan, Yuandeng Shen, Hechao Chen +4
Solar macrospicules are beam-like cool plasma ejections of size in-between spicules and coronal jets, which can elucidate potential connections between plasma jetting activity at d…
Recurrent narrow quasi-periodic fast-propagating wave trains excited by the intermittent energy release in the accompanying solar flare
Xinping Zhou, Yuandeng Shen, Hongfei Liang +5
About the driven mechanisms of the quasi-periodic fast-propagating (QFP) wave trains, there exist two dominant competing physical explanations: associated with the flaring energy r…
White-light QFP Wave Train and the Associated Failed Breakout Eruption
Yuandeng Shen, Surui Yao, Zehao Tang +5
Quasi-periodic fast-propagating (QFP) magnetosonic wave trains are commonly observed in the low corona at extreme ultraviolet wavelength bands. Here, we report the first white-ligh…
Stereoscopic diagnosing of a filament-cavity flux rope system by tracing the path of a two-sided-loop jet
Song Tan, Yuandeng Shen, Xinping Zhou +4
The fine magnetic structure is vitally important to understanding the formation, stabilization and eruption of solar filaments, but so far, it is still an open question yet to be r…
Observations of a Flare-ignited broad Quasi-periodic Fast-propagating wave train
Xinping Zhou, Yuandeng Shen, Ying D. Liu +6
Large-scale Extreme-ultraviolet (EUV) waves are frequently observed as an accompanying phenomenon of flares and coronal mass ejections (CMEs). Previous studies mainly focus on EUV…
Homologous Accelerated Electron Beams, Quasi-periodic fast-propagating Wave and CME Observed in one Fan-spine Jet
Yadan Duan, Yuandeng Shen, Xinping Zhou +3
Using imaging and radio multi-wavelength observations, we studied the origin of two homologous accelerated electron beams and a quasi-periodic fast-propagating (QFP) wave train ass…
Total reflection of a flare-driven quasi-periodic EUV wave train at a coronal hole boundary
Xinping Zhou, Yuandeng Shen, Zehao Tang +3
The reflection, refraction, and transmission of large-scale extreme ultraviolet (EUV) waves (collectively, secondary waves) have been observed during their interactions with corona…
Coronal Quasi-periodic Fast-mode Propagating Wave Trains
Yuandeng Shen, Xinping Zhou, Yadan Duan +3
QFP wave trains in the corona have been studied intensively in the past decade, thanks to the full-disk, high spatiotemporal resolution, and wide-temperature coverage observations…
Sympathetic Filament Eruptions within a Fan-spine Magnetic System
Chengrui Zhou, Yuandeng Shen, Xinping Zhou +3
It is unclear whether successive filament eruptions at different sites within a short time interval are physically connected or not. Here, we present the observations of the succes…
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Successively Detected in a Solar Eruption
Xinping Zhou, Yuandeng Shen, Jiangtao Su +4
We present SDO/AIA observation of three types of fast-mode propagating magnetosonic waves in a GOES C3.0 flare on 2013 April 23, which was accompanied by a prominence eruption and…
Sympathetic Standard and Blowout Coronal Jets Observed in a Polar Coronal Hole
Zehao Tang, Yuandeng Shen, Xinping Zhou +4
We present the sympathetic eruption of a standard and a blowout coronal jets originating from two adjacent coronal bright points (CBP1 and CBP2) in a polar coronal hole, using soft…
Direct Observation of A Large-scale CME Flux Rope Event Arising from an Unwinding Coronal Jet
Hechao Chen, Jiayan Yang, Junchao Hong +2
Coronal mass ejections (CMEs) and coronal jets are two types of common solar eruptive phenomena, which often independently happen at different spatial scales. In this work, we pres…
Round-trip Slipping Motion of the Circular Flare Ribbon Evidenced in a Fan-spine Jet
Yuandeng Shen, Zhining Qu, Chengrui Zhou +3
A solar jet on 2014 July 31, which was accompanied by a GOES C1.3 flare and a mini-filament eruption at the jet base, was studied by using observations taken by the New Vacuum Sola…