activity
20232026
most citedHigh-resolution Observations of a C9.3 White-light Flare and Its Impact on the Solar Photosphere

6 citations · 14 across the 12 of their papers we have counts for

collaborators

13 papers

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.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

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.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…