collaborators

10 papers

astro-ph.SR2026

Double-periodic pulsations simultaneously detected in mid-infrared and hard X-ray emissions during an X1.5 flare

Dong Li, Yuyang Ye, Xianyong Bai +1

Quasi-periodic pulsations (QPPs) have been observed in a broad electromagnetic spectrum, encompassing radio, ultraviolet, white light, X-rays, and Gama-rays. Yet, flare-associated…

astro-ph.SR2026

Detection and analysis of white-light emission in solar flares through light curve diagnostics

Shuanghong Li, Yongliang Song, Kun Wang +4

White-light flares (WLFs) are crucial for understanding the energy transport and heating processes in the lower solar atmosphere. Systematic studies are highly necessary. However,…

astro-ph.SR2026

Magnetic Field Measurements in the Solar Chromosphere Using the H 4861Ã ~Line I: Forward Modeling Based on 1D Models

Jiasheng Wang, Wenxian Li, Xianyong Bai +3

The chromosphere is a complex solar atmosphere that hosts a variety of transients and transports significant free energy to heat the corona. However, due to the limited sensitivity…

astro-ph.SR2025

The First Scientific Flight and Observations of the 50-mm Balloon-Borne White-Light Coronagraph

Kaifeng Kang, Min Huang, Yang Liu +13

A 50-mm balloon-borne white-light coronagraph (BBWLC) to observe whitelight solar corona over the altitude range from 1.08 to 1.50 solar radii has recently been indigenously develo…

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…

astro-ph.SR2025

Characterization and formation of the Mg i 12.32 μm line in the quiet Sun and sunspot

Yuchuan Wu, Wenxian Li, Xianyong Bai +3

The Mg I 12.32 μm line is highly sensitive to magnetic fields due to its long wavelength, making it a promising tool for precise solar-magnetic-field measurements. The formation o…