activity
20132026
most citedSimultaneous observation of a flux rope eruption and magnetic reconnection during an X-class solar flare

121 citations · 569 across the 33 of their papers we have counts for

collaborators

35 papers

astro-ph.SR2026

High-Frequency Transverse Waves in Chromospheric Fibrils Revealed by DKIST

Qifan Dong, Xiaoli Yan, Zhike Xue +4

Chromospheric fibrils are ubiquitous dynamical structures that can support magnetohydrodynamic waves and may contribute to energy transport in the solar atmosphere. Using high-reso…

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

Observational Evidence of Solar Spicules Associated with Microfilament Eruptions Using DKIST

Qifan Dong, Xiaoli Yan, Zhike Xue +8

The formation mechanism of spicules is fundamentally important for understanding mass and energy transport from the chromosphere into the corona. Recent studies suggested that spic…

astro-ph.SR2026

Spectroscopic Case Studies of Four Long-duration Transition-region Explosive Events

Yi'an Zhou, Xiaoli Yan, Zhike Xue +3

This work presents a detailed spectroscopic case study of four long-duration transition-region (TR) explosive events (EEs) observed in NOAA Active Region 13213 on 2023 February 10…

astro-ph.SR2026

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…

astro-ph.SR2025

Observational study of chromospheric jets in and around a sunspot observed by NVST and SDO

Guotang Wu, Xiaoli Yan, Zhike Xue +8

To better understand the characteristics, driving mechanisms, and potential heating contributions of chromospheric jets, we analyze two contrasting types: one originating from with…

astro-ph.SR2025

Properties of Chromospheric Fibrils Around a Quiescent Filament

Qifan Dong, Xiaoli Yan, Zhike Xue +7

Fibrils are dynamic plasma structures in the solar chromosphere. Studying these structures is critical for understanding solar atmospheric heating and mass transportation. The purp…

astro-ph.SR2025★ 6 cited

High-resolution Observations of a C9.3 White-light Flare and Its Impact on the Solar Photosphere

Zhe Xu, Xiaoli Yan, Zhentong Li +4

We present a detailed analysis of a C9.3 white-light flare using high-resolution observations from the New Vacuum Solar Telescope (NVST). The flare occurred near the eastern solar…

astro-ph.SR2025★ 2 cited

The Observations of Magnetic Reconnection During the Interaction Process of Two Active Region Filaments

Zongyin Wu, Zhike Xue, Xiaoli Yan +11

We investigate the interaction between two filaments (F1 and F2) and their subsequent magnetic reconnection in active region (AR) NOAA 13296 and AR NOAA 13293 on May 9, 2023, utili…

astro-ph.SR2025

Recurrent Jetlets Associated with the Disappearance of a Satellite Spot

Liheng Yang, Xiaoli Yan, Jun Zhang +10

Recurrent small-scale eruptions are fascinating phenomena in the solar atmosphere. However, their underlying physical mechanisms remain unclear. On 2021 May 23, five recurrent jetl…

astro-ph.SR2025

Simultaneous existence of the ocsillations, counterstreaming flows and mass injections in solar quiescent prominences

X. L. Yan, Z. K. Xue, J. C. Wang +8

Solar prominences are very spectacular structures embedded in the tenuous and hot solar corona. The counterstreaming flows, a common feature in solar quiescent prominences, have be…

astro-ph.SR2024★ 1 cited

Variation in the intensity ratio at each wavelength point of the Si iv 1394/1403 Å lines. Spectral diagnostics of a bifurcated eruption

Yi'an Zhou, Xiaoli Yan, Zhike Xue +3

Aims. This study aims to investigate the deviation of the intensity ratio of the \ion{Si}{IV} 1394 Å and 1403 Å emission lines from the expected value of 2 in the optically thin re…

astro-ph.SR2024

The hidden magnetic structures of a solar intermediate filament revealed by the injected flare material

X. L. Yan, Z. K. Xue, J. C. Wang +7

Solar filaments are spectacular objects in the solar atmosphere, consisting of accumulations of cool, dense, and partially ionized plasma suspended in the hot solar corona against…

astro-ph.SR2024★ 1 cited

Origin of the Chromospheric Umbral Waves in Sunspots

Xinsheng Zhang, Xiaoli Yan, Zhike Xue +5

Oscillations are ubiquitous in sunspots and the associated higher atmospheres. However, it is still unclear whether these oscillations are driven by the external acoustic waves (p-…

astro-ph.SR2024

Negative-energy waves in the vertical threads of a solar prominence

Jincheng Wang, Dong Li, Chuan Li +5

Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination due to their thread-like features and dynamic behaviors. Utilizing data from the New V…

astro-ph.SR2024

Imaging and spectroscopic observations of a confined solar filament eruption with two-stage evolution

Zhe Xu, Xiaoli Yan, Liheng Yang +3

Solar filament eruptions are often characterized by stepwise evolution due to the involvement of multiple mechanisms, such as magnetohydrodynamic instabilities and magnetic reconne…

astro-ph.SR2024★ 5 cited

The Decay of Two Adjacent Sunspots Associated with Moving Magnetic Features

Yang Peng, Zhike Xue, Zhongquan Qu +4

The relationship between the decay of sunspots and moving magnetic features (MMFs) plays an important role in understanding the evolution of active regions. We present observations…

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

Onset mechanism of an inverted U-shaped solar filament eruption revealed by NVST, SDO, and STEREO-A observations

Jincheng Wang, Xiaoli Yan, Qiangwei Cai +10

Utilizing observations from the New Vacuum Solar Telescope (NVST), Solar Dynamics Observatory (SDO), and Solar Terrestrial Relations Observatory-Ahead (STEREO-A), we investigate th…

astro-ph.SR2020★ 20 cited

Dynamics evolution of a solar active-region filament from quasi-static state to eruption: rolling motion, untwisting motion, material transfer, and chirality

X. L. Yan, Q. L. Li, G. R. Chen +5

To better understand magnetic structure and eruptive process of solar filaments, a solar active-region filament (labeled F2) eruption associated with a B-class flare was investigat…

astro-ph.SR2020★ 16 cited

A small-scale filament eruption inducing Moreton Wave, EUV Wave and Coronal Mass Ejection

Jincheng Wang, Xiaoli Yan, Defang Kong +3

With the launch of SDO, many EUV waves were observed during solar eruptions. However, the joint observations of Moreton and EUV waves are still relatively rare. We present an event…

astro-ph.SR2019★ 6 cited

The formation and decay of sunspot penumbra in Active Region NOAA 12673

Qiaoling Li, Xiaoli Yan, Jincheng Wang +3

To better understand the formation and decay of sunspot penumbra, we studied the evolution of sunspots in the three regions of the active-region NOAA 12673 in detail. The evolution…

astro-ph.SR2019★ 29 cited

Formation and material supply of an active-region filament associated with newly emerging flux

Jincheng Wang, Xiaoli Yan, 2Qiaoling Guo +4

With the observations of SDO/AIA 304 Å and NVST Hα bands, we present the formation process of an active-region filament in active region NOAA 11903 during the period from 02:00 UT…

astro-ph.SR2018★ 14 cited

The initial morphologies of the wavefronts of extreme ultraviolet waves

Ruisheng Zheng, Zhike Xue, Yao Chen +2

The morphologies of the wavefronts of extreme ultraviolet (EUV) waves can shed light on their physical nature and driving mechanism that are still strongly debated. In reality, the…