activity
20112025
most citedA fundamental mechanism of solar eruption initiation

156 citations · 930 across the 34 of their papers we have counts for

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Showing astro-ph.SRShow all

35 papers · 1 filter

astro-ph.SR2025

High-Resolution Observation of Solar Prominence Plumes Induced by Enhanced Spicular Activity

Wensi Wang, Rui Liu, Runbin Luo +1

Solar prominences are the most prominent large-scale structures observed above the solar limb in emission in chromospheric lines but in absorption in coronal lines. At the bottom o…

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

Tracking an eruptive intermediate prominence originating from the farside of the Sun

Qingmin Zhang, Wenwei Pan, Beili Ying +7

In this paper, we carry out multiwavelength and multiview observations of the eruption of an intermediate prominence originating from the farside of the Sun on 2023 March 12. The s…

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

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

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★ 2 cited

Magnetic Reconnection as the Key Mechanism in Sunspot Rotation Leading to Solar Eruption

Chaowei Jiang, Xueshang Feng, Xinkai Bian +8

The rotation of sunspots around their umbral center has long been considered as an important process in leading to solar eruptions, but the underlying mechanism remains unclear. A…

astro-ph.SR2023

Data-driven MHD simulation of a sunspot rotating active region leading to solar eruption

Chaowei Jiang, Xueshang Feng, Xinkai Bian +8

Solar eruptions are the leading driver of space weather, and it is vital for space weather forecast to understand in what conditions the solar eruptions can be produced and how the…

astro-ph.SR2022★ 21 cited

Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere

Yuming Wang, Xianyong Bai, Changyong Chen +50

Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360° perspective in the ecliptic plane. It will deploy three 120…

astro-ph.SR2021★ 156 cited

A fundamental mechanism of solar eruption initiation

Chaowei Jiang, Xueshang Feng, Rui Liu +8

Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are initiated remains unclear. Prevailing theories often rely on special magnetic topologies t…

astro-ph.SR2021★ 7 cited

Naked emergence of an anti-Hale active region I. Overall evolution and magnetic properties

Jincheng Wang, Xiaoli Yan, Defang Kong +5

{In order to understand the emergence of the active region, we investigate the emerging process and magnetic properties of a naked anti-Hale active region during the period between…

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★ 46 cited

Triggering mechanism and material transfer of a failed solar filament eruption

X. L. Yan, Z. K. Xue, X. Cheng +6

Soar filament eruptions are often associated with solar flares and coronal mass ejections (CMEs), which are the major impacts on space weather. However, the fine structures and the…

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

Energy origination and triggering mechanism of a series of homologous confined flares

Guorong Chen, Xiaoli Yan

Using the H data from the New Vacuum Solar Telescope (NVST) at the Fuxian Solar Observatory together with multi-wavelength images and magnetograms obtained by Solar Dynamics Obs…

astro-ph.SR2019★ 1 cited

Research progress based on observations of the New Vacuum Solar Telescope

Xiaoli Yan, Zhong Liu, Jun Zhang +1

The purpose of this paper is to introduce the main scientific results made by the one-meter New Vacuum Solar Telescope (NVST), which was put into commission on 2010. NVST is one of…

astro-ph.SR2019★ 14 cited

Properties of local oscillations in the lower sunspot atmosphere

Robert Sych, Yuzef Zhugzhda, Xiaoli Yan

We present a study of wave processes in the sunspot region NOAA 12670 on 2017 August 10 observed by the Goode Solar Telescope in the TiO 7057 A and Ha 6563 A spectral lines. To stu…

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★ 38 cited

Formation of an active region filament driven by a series of jets

Jincheng Wang, Xiaoli Yan, ZhongQuan Qu +5

We present a formation process of a filament in active region NOAA 12574 during the period from 2016 August 11 to 12. Combining the observations of GONG H, Hida spectrum and SDO…

astro-ph.SR2018★ 106 cited

Successive X-class flares and coronal mass ejections driven by shearing motion and sunspot rotation in active region NOAA 12673

X. L. Yan, J. C. Wang, G. M. Pan +5

We present a clear case study on the occurrence of two successive X-class flares including a decade-class flare (X9.3) and two coronal mass ejections (CMEs) triggered by shearing m…