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6 papers

astro-ph.IM2026

Design and Implementation of a Microservice-Architecture Master Control System for AIMS

Li-Yue Tong, Jia-Ben Lin, Jun-Feng Hou +11

The paper presents a microservice‑based Master Control System that automates the AIMS solar infrared telescope, using a layered architecture and autonomous functions like pointing,…

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

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…

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.SR2025

Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament

Hechao Chen, Hui Tian, Quanhao Zhang +8

Filament eruptions are magnetically driven violent explosions commonly observed on the Sun and late-type stars, sometimes leading to monster coronal mass ejections that directly af…