207 citations · 2.4k across the 65 of their papers we have counts for
65 papers
Solar Orbiter reveals persistent magnetic reconnection in medium-scale filament eruptions
Song Tan, Alexander Warmuth, Frédéric Schuller +7
Solar filament eruptions play a key role in driving space weather, yet their fine-scale evolution remains poorly understood due to observational limitations. Using unprecedented hi…
Extremely diverse coronal jets accompanying an erupting filament captured by Solar Orbiter
Song Tan, Alexander Warmuth, Frédéric Schuller +3
Solar jets are collimated plasma ejections driven by magnetic reconnection, which play a critical role in the energy release and mass transport in the solar atmosphere. Using Solar…
From Photospheric Footpoint Motion to Plasmoid Ejection: A Two-Stage Reconnection Process in a Small-scale Chromospheric Jet
Zehao Tang, Yuandeng Shen, Chengrui Zhou +3
Using high spatiotemporal resolution, multi-wavelength observations from the New Vacuum Solar Telescope (NVST) and the Solar Dynamics Observatory (SDO), we present a detailed analy…
How Reconnection-Unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions
Chengrui Zhou, Yuandeng Shen, Chun Xia +4
Magnetic flux emergence is traditionally considered a key trigger of solar filament eruptions; however, its role in suppressing filament eruptions remains less understood. Using mu…
Deciphering the Formation and Dynamics of Double-decker Filament Through Component Magnetic Reconnection
Dongxu Liu, Yuandeng Shen, Yi Bi +3
The formation of double-decker filaments has long been an enigma in the field of solar physics. Using stereoscopic observations from the Solar Dynamics Observatory and the Solar Te…
High-Resolution Observations of a Small-Scale Cancellation Nanoflare: Supporting Evidence for the Cancellation Nanoflare Model
Zehao Tang, Yuandeng Shen, Chengrui Zhou +2
An analytical cancellation nanoflare model has recently been established to show the fundamental role that ubiquitous small-scale cancellation nanoflares play in solar atmospheric…
A New Formation Mechanism of Counterstreaming Mass Flows in Filaments and the Doppler Bullseye Pattern in Prominences
Chengrui Zhou, Yuandeng Shen, Chun Xia +3
The eruption of solar prominences can eject substantial mass and magnetic field into interplanetary space and cause geomagnetic storms. However, various questions about prominences…
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…
Formation and Eruption of Hot Channel Magnetic Flux Rope in Nested Double Null Magnetic System
Surui Yao, Yuandeng Shen, Chengrui Zhou +2
The coronal magnetic topology significantly affects the outcome of magnetic flux rope (MFR) eruptions. The recently reported nested double null magnetic system remains unclear as t…
On the origin of a broad QFP wave train: unwinding jet as the driver
Xinping Zhou, Zehao Tang, Zhining Qu +5
Large-scale extreme-ultraviolet (EUV) waves commonly exhibit as single wavefront and are believed to be caused by coronal mass ejections (CMEs). Utilizing high spatiotemporal resol…
Formation and Evolution of Transient Prominence Bubbles Driven by Erupting Mini-filaments
Yilin Guo, Yijun Hou, Ting Li +6
Prominence bubbles, the dark arch-shaped "voids" below quiescent prominences, are generally believed to be caused by the interaction between the prominences and the slowly-emerging…
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…
Broad and Bi-directional narrow quasi-periodic fast-propagating wave trains associated with a filament-driven halo CME on 2023 April 21
Xinping Zhou, Yuandeng Shen, Yihua Yan +8
This paper presents three distinct wave trains that occurred on 2023 April 21: a broad quasi-periodic fast-propagating (QFP) wave train and a bi-directional narrow QFP wave train.…
Resolved magnetohydrodynamic wave lensing in the solar corona
Xinping Zhou, Yuandeng Shen, Ding Yuan +6
Electromagnetic wave lensing, a common physical phenomenon recognized in visible light for centuries, finds extensive applications in manipulating light in optical systems such as…
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…
Consecutive Narrow and Broad Quasi-periodic Fast-propagating Wave Trains Associated with a Flare
Xinping Zhou, Yuandeng Shen, Chengrui Zhou +2
The excitation mechanism of coronal quasi-period fast-propagating (QFP) wave trains remains unresolved. Using Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory ob…
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…
Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere
Yuming Wang, Xianyong Bai, Changyong Chen +50
Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360° perspective in the ecliptic plane. It will deploy three 120…
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…