activity
20102025
most citedOn a Coronal Blowout Jet: The First Observation of a Simultaneously Produced Bubble-like CME and a Jet-like CME in a Solar Event

207 citations · 2.4k across the 65 of their papers we have counts for

collaborators
Showing 2024Show all

10 papers · 1 filter

astro-ph.SR2024

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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.…

astro-ph.SR2024★ 26 cited

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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…