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20232026
most citedResolving Interchange Reconnection Dynamics in a Fan-Spine-like Topology Observed by Solar Orbiter

3 citations · 3 across the 14 of their papers we have counts for

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astro-ph.SR2026

Intense but Harmless: Exo-Space Weather Around an M Dwarf with a Single-Hemisphere Dynamo

Zheng Sun, Julián D. Alvarado-Gómez, Hui Tian +4

M dwarfs are among the most promising host stars in the search for habitable exoplanets. However, their active atmospheres drive intense magnetic activity, including energetic flar…

astro-ph.SR2026

How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics

Zheng Sun, Julián D. Alvarado-Gómez, Hui Tian

Observations show that stellar coronal mass ejection (CME) candidates display relatively lower kinetic energies compared to expectations from solar flare-CME relations extrapolated…

astro-ph.SR2026

Fine-scale downflows above flare ribbons captured by Solar Orbiter/EUI

Zheng Sun, Alexander G. M. Pietrow, Malcolm K. Druett +8

In solar flares, flare ribbons map chromospheric footpoints where flare energy deposition occurs. These locations are associated with field aligned energy transport from the corona…

astro-ph.SR2026

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…

astro-ph.SR2025★ 3 cited

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…

astro-ph.SR2025

The Detectability of Coronal Mass Ejections in the Low Corona Using Multi-slit Extreme-ultraviolet Spectroscopy

Lami Chan, Xianyong Bai, Hui Tian +6

The spectra of coronal mass ejections (CMEs) in the low corona play a crucial role in understanding their origins and physical mechanism, and enhancing space weather forecasting. H…

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

An Extreme Stellar Prominence Eruption Observed by LAMOST Time-Domain Spectroscopy

Lu Hong-Peng, Tian Hui, Zhang Li-Yun +6

We report the detection of an extreme stellar prominence eruption on the M dwarf LAMOST J044431.62+235627.9, observed through time-domain H spectroscopy with the Large Sky Area…

astro-ph.SR2024

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…

astro-ph.SR2024

Three types of solar coronal rain during magnetic reconnection between open and closed magnetic structures

Fangfang Qiao, Leping Li, Hui Tian +4

Coronal rain (CR) is a crucial part of the mass cycle between the corona and chromosphere. It includes the flare-driven CR and two types of quiescent CR separately along the non-fl…

astro-ph.SR2024

The Solar Origin of an Intense Geomagnetic Storm on 2023 December 1st: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes

Zheng Sun, Ting Li, Yijun Hou +12

The solar eruption that occurred on 2023 November 28 (SOL2023-11-28) triggered an intense geomagnetic storm on Earth on 2023 December 1. The associated Earth's auroras manifested a…

astro-ph.SR2024

Is it possible to detect coronal mass ejections on solar-type stars through extreme-ultraviolet spectral observations?

Zihao Yang, Hui Tian, Yingjie Zhu +3

Stellar coronal mass ejections (CMEs) from host stars are an important factor that affects the habitability of exoplanets. Although their solar counterparts have been well observed…

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.SR2023

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…