activity
20242026
collaborators

6 papers

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.SR2026

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

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

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…