collaborators

5 papers

astro-ph.SR2026

Research Progress on Solar Small-Scale Dynamo

Wen-Jie Jiang, Lei Ni, Chun-Lan Jin +2

The small-scale solar dynamo theory, as the core mechanism explaining the origin of the persistent, disperse weak magnetic field in the quiet Sun regions, has made significant prog…

astro-ph.SR2025

QFP Waves Driven by the Tuning-Fork Effect during Magnetic Reconnecion

Jialiang Hu, Xiaozhou Zhao, Guiping Zhou +8

Through three-dimensional MHD simulations, we have uncovered a kind of fast coronal wave originating from both ends of a current sheet (CS) during a solar eruption. These waves are…

astro-ph.SR2025

Variations of the vector magnetic structures in the solar polar regions observed by Hinode

Shuhong Yang, Chunlan Jin, Qiao Song +7

Using the polar vector magnetic field data observed by Hinode from 2012 to 2021, we study the long-term variations of the magnetic flux, the flux proportion of different polarities…

astro-ph.SR2025

Probing Solar Polar Regions

Yuanyong Deng, Hui Tian, Jie Jiang +45

The magnetic fields and dynamical processes in the solar polar regions play a crucial role in the solar magnetic cycle and in supplying mass and energy to the fast solar wind, ulti…

astro-ph.SR2025

Atmospheric Heating Events Associated with Fine-scale Flux Emergence in Ephemeral Regions

Hanlin Yang, Jingxiu Wang, Chunlan Jin

Coronal heating has puzzled solar physicists for decades. The question of why the Sun's upper atmosphere is significantly hotter than its lower atmosphere remains a key mystery. It…