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20232025
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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.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

Heating Mechanisms and Radio Response from the Solar Chromosphere to Corona

Baolin Tan, Jing Huang, Yin Zhang

Heating mechanism in the solar atmosphere (from chromosphere to corona) is one of the top-challenges in modern astronomy. The classic mechanisms can be divided into two categories:…

astro-ph.SR2025

The occurrence of powerful flares stronger than X10 class in Solar Cycles

Baolin Tan, Yin Zhang, Jing Huang +1

Solar flares stronger than X10 (S-flares, >X10) are the highest class flares which significantly impact on the Sun's evolution and space weather. Based on observations of Geostatio…

astro-ph.SR2024

Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops

Leping Li, Hongqiang Song, Yijun Hou +11

Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…

astro-ph.SR2023

The physics of solar spectral imaging observations in dm-cm wavelengths and the application on space weather

Baolin Tan, Yihua Yan, Jing Huang +3

Recently, several new solar radio telescopes have been put into operation and provided spectral-imaging observations with much higher resolutions in decimeter (dm) and centimeter (…