activity
20122026
most citedSolar Filament Recognition Based on Deep Learning

35 citations · 68 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.IM2026

Graph Learning with Multiplicative Aggregation for Solar Filament Fragment Association Modeling in Full-disk H Images

GaoFei Zhu, GangHua Lin, Xiao Yang +4

Solar filaments are prominent features in H observations. During their evolution, they often exhibit complex morphological and topological changes, which, due to line-of-sight p…

astro-ph.SR2026

Oscillation Period Properties of Sunspots in the 8-10 m Infrared Band: A Multi-Dataset Analysis

Suo Liu

Sunspot oscillations probe magnetic-plasma interactions in the solar atmosphere. We investigate oscillation periods in six sunspot active regions observed in the 8-10 um band with…

astro-ph.SR2026

JW-VL: A Vision-Language Model for Solar Physics

Mingfu Shao, Hui Wang, Liyue Tong +7

Vision-Language Models (VLMs) have achieved breakthrough progress in general knowledge domains, yet adaptation to specialized scientific fields remains challenging due to multimoda…

astro-ph.SR2025

JW-Flare: Accurate Solar Flare Forecasting Method Based on Multimodal Large Language Models

Mingfu Shao, Hui Wang, Yuyang Li +17

Solar flares, the most powerful explosive phenomena in the solar system, may pose significant hazards to spaceborne satellites and ground-based infrastructure. Despite decades of i…

astro-ph.SR2025★ 2 cited

Advances and Challenges in Solar Flare Prediction: A Review

Mingfu Shao, Suo Liu, Haiqing Xu +8

Solar flares, as one of the most prominent manifestations of solar activity, have a profound impact on both the Earth's space environment and human activities. As a result, accurat…

astro-ph.SR2025

Responses of a Coronal Hole to a Fast Flare-Driven Coronal Wave

Xiaofan Zhang, Huadong Chen, Guiping Zhou +12

Coronal waves, significant solar phenomena, act as diagnostic tools for scientists studying solar atmosphere properties. Here, we present a novel observation detailing how a corona…

astro-ph.SR2024

Comparison of Relative Magnetic Helicity Flux Calculation Results Based on the Line-of-Sight Magnetograms of ASO-S/FMG and SDO/HMI

Shangbin Yang, Suo Liu, Jiangtao Su +1

Magnetic helicity is a key geometrical parameter to describe the structure and evolution of solar coronal magnetic fields. The accumulation of magnetic helicity is correlated with…

astro-ph.SR2024

Correction for the Weakening Magnetic Field within the Sunspot Umbra Observed by ASO-S/FMG

Haiqing Xu, Jiangtao Su, Suo Liu +6

The magnetic field inside the sunspot umbra, as observed by the Full-disk MagnetoGraph (FMG) onboard the Advanced Space based Solar Observatory (ASO-S), was found to be experiencin…

astro-ph.SR2024

Observation of a large-scale filament eruption initiated by two small-scale erupting filaments pushing out from below

Yongliang Song, Jiangtao Su, Qingmin Zhang +9

Filament eruptions often result in flares and coronal mass ejections (CMEs). Most studies attribute the filament eruptions to their instabilities or magnetic reconnection. In this…

astro-ph.SR2020★ 7 cited

Automatic Detection and Correction Algorithms for Magnetic Saturation in the SMFT/HSOS longitudinal Magnetograms

Haiqing Xu, Suo Liu, Jiangtao Su +8

longitudinal magnetic field often suffers the saturation effect in strong magnetic field region when the measurement performs in a single-wavelength point and linear calibration is…

astro-ph.SR2020★ 11 cited

A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I

GangHua Lin, GaoFei Zhu, Xiao Yang +12

Filaments are very common physical phenomena on the Sun and are often taken as important proxies of solar magnetic activities. The study of filaments has become a hot topic in the…

astro-ph.IM2019★ 35 cited

Solar Filament Recognition Based on Deep Learning

GaoFei Zhu, GangHua Lin, DongGuang Wang +2

The paper presents a reliable method using deep learning to recognize solar filaments in H-alpha full-disk solar images automatically. This method cannot only identify filaments ac…

astro-ph.SR2019

Standard Magnetic Field Production at Huairou Solar Observing Station

Suo Liu, Ganghua Lin, Xiao Yang +3

The regular solar observations are operated at Huairou Solar Observing Station (HSOS) since 1987, which make the construction of long-term magnetic field datasets available to unde…

astro-ph.SR2019★ 1 cited

Energy Build-up and Triggering Leading to a M1.5 Flare on 1 August 2014

S. Liu, J. T. Su

The energy storage and trigger mechanisms of solar flares are important for understanding of solar activity. We analyzed multi-wavelength observations of a M1.5 flare on 1 August 2…

astro-ph.SR2018★ 2 cited

Super Penumbral Chromospheric Flare

S. Liu, H. Q. Zhang, D. P. Choudhary +2

We observed a C-class flare at the outer boundary of the super-penumbra of a sunspot. The flare was triggered by an emerging magnetic bipolar region that was obliquely oriented wit…

astro-ph.SR2014★ 1 cited

A Statistical Study on Property of Spatial Magnetic Field for Solar Active Region

Suo Liu

Magnetic fields dominate most solar activities, there exist direct relations between solar flare and the distributions of magnetic field, and also its corresponding magnetic energy…

astro-ph.SR2012★ 9 cited

A Coronal Jet Ejects from Sunspot Light Bridge

Suo Liu

Chromospheric brighten and H surge are the evident and common phenomena along sunspot light bridge. In this paper, a coronal jet ejects from sunspot light bridge is presented. U…