activity
20182025
most citedRecurrent Two-Sided Loop Jets Caused by Magnetic Reconnection between Erupting Minifilaments and Nearby Large Filament

36 citations · 203 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2025

Multiwavelength Observations for a Double-decker Filament Channel in AR 13102

Yin Zhang, Baolin Tan, Quan Wang +8

We present the observational evidence of the existence of a double-decker filament channel (FC) by using observations in extreme ultraviolet and Hα wavelengths. For both FCs, the e…

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★ 1 cited

The Decay Process of an α-configuration Sunspot

Yang Peng, Zhi-Ke Xue, Xiao-Li Yan +8

The decay of sunspot plays a key role in magnetic flux transportation in solar active regions (ARs). To better understand the physical mechanism of the entire decay process of a su…

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.SR2023★ 8 cited

Morphological evidence for nanoflares heating warm loops in the solar corona

Y. Bi, J. J. Yang, Y. Qin +6

Nanoflares are impulsive energy releases by magnetic reconnection in the braided coronal magnetic field, which is a potential mechanism for heating the corona. However, there are s…

astro-ph.SR2022★ 15 cited

Reconfiguration and eruption of a solar filament by magnetic reconnection with an emerging magnetic field

Leping Li, Hardi Peter, Lakshmi Pradeep Chitta +3

Both observations and simulations suggest that the solar filament eruption is closely related to magnetic flux emergence. It is thought that the eruption is triggered by magnetic r…

astro-ph.SR2022★ 4 cited

Sunspot shearing and sudden retraction motion associated with the 2013 August 17 M3.3 Flare

Yanjie Zhang, Zhe Xu, Qingmin Zhang +2

In this Letter, we give a detailed analysis to the M3.3 class flare that occurred on August 17, 2013 (SOL2013-08-17T18:16). It presents a clear picture of mutual magnetic interacti…

astro-ph.SR2022★ 19 cited

Statistical analysis of circular-ribbon flares

Yanjie Zhang, Qingmin Zhang, Dechao Song +4

Circular-ribbon flares (CFs) are a special type of solar flares owing to their particular magnetic topology. In this paper, we conducted a comprehensive statistical analysis of 134…

astro-ph.SR2022★ 19 cited

A partial filament eruption in three steps induced by external magnetic reconnection

Jun Dai, Zhentong Li, Ya Wang +6

We present an investigation of partial filament eruption on 2012 June 17 in the active region NOAA 11504. For the first time, we observed the vertical splitting process during the…

astro-ph.SR2021★ 25 cited

Formation of a Solar Filament by Magnetic Reconnection and Associated Chromospheric Evaporation and Subsequent Coronal Condensation

Bo Yang, Jiayan Yang, Yi Bi +2

We present the first observation of a solar filament formed by magnetic reconnection and associated chromospheric evaporation and subsequent coronal condensation. Driven by shearin…

astro-ph.SR2021★ 26 cited

Oscillations and mass-draining that lead to a sympathetic eruption of a quiescent filament

Jun Dai, Qingmin Zhang, Yanjie Zhang +3

In this paper, we present a multi-wavelength analysis to mass-draining and oscillations in a large quiescent filament prior to its successful eruption on 2015 April 28. The eruptio…

astro-ph.SR2021★ 5 cited

Recurrent coronal jets observed by SDO/AIA

Yan-Jie Zhang, Qing-Min Zhang, Jun Dai +2

In this paper, we carry out multiwavelength observations of three recurring jets on 2014 November 7. The jets originated from the same region at the edge of AR 12205 and propagated…

astro-ph.SR2021★ 8 cited

Magneto-acoustic oscillations observed in a solar plage region

Haisheng Ji, Parida Hashim, Zhenxiang Hong +4

We gave an extensive study for the quasi-periodic perturbations on the time profiles of the line of sight (LOS) magnetic field in 10x10 sub-areas in a solar plage region (correspon…

astro-ph.SR2019★ 36 cited

Recurrent Two-Sided Loop Jets Caused by Magnetic Reconnection between Erupting Minifilaments and Nearby Large Filament

Bo Yang, Jiayan Yang, Yi Bi +4

Using high spatial and temporal data from the New Vacuum Solar Telescope (NVST) and the Solar Dynamics Observatory (SDO), we present unambiguous observations of recurrent two-sided…

astro-ph.SR2018★ 12 cited

A Survey of Changes in Magnetic Helicity Flux on the Photosphere During Relatively Low Class Flares

Yi Bi, Ying D Liu, Yanxiao Liu +3

Using the 135-second cadence of the photospheric vector data provided by the Helioseismic and Magnetic Imager telescope on board the Solar Dynamic Observatory, we examined the time…

astro-ph.SR2018★ 20 cited

Observational Evidence of Magnetic Reconnection Associated with Magnetic Flux Cancellation

Bo Yang, Jiayan Yang, Yi Bi +4

Using high spatial and temporal data from the \emph{Solar Dynamics Observatory} (\emph{SDO}) and the \emph{Interface Region Imaging Spectrograph} (\emph{IRIS}), several observation…