collaborators

6 papers

astro-ph.EP2025

A High-Precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multi-Layer Internal Structure Models

Kai Huang, Yongzhang Yang, Yuhao Chen +2

China is planing to launch the Tianwen-4 mission around the year 2030, with its aim being the exploration of Jupiter and its moon, Callisto. Within the realm of deep space explorat…

astro-ph.SR2025

Coronal Mass Ejections Deflected by Newly Emerging Flux: A Combined Analytic and Numerical Study

Yuhao Chen, Chengcai Shen, Zhixing Mei +8

Newly emerging flux (NEF) has been widely studied as a trigger of solar filament eruptions, but its influence on the subsequent dynamics remains poorly explored. Because NEF typica…

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

Numerical simulation of oscillatory magnetic reconnection modulated by solar convective motions

Yifu Wang, Lei Ni, Guanchong Cheng +3

Oscillatory magnetic reconnection is a periodic magnetic reconnection process, during which the current sheet's orientation and the magnetic connections change periodically. This p…

astro-ph.SR2024

Components and anisotropy of 3D QFP waves during the early solar eruption

Jialiang Hu, Jing Ye, Yuhao Chen +3

The propagation of disturbances in the solar atmosphere is inherently three dimensional (3D), yet comprehensive studies on the spatial structure and dynamics of 3D wavefronts are s…

astro-ph.SR2024

Theoretical Studies on the Evolution of Solar Filaments in Response to New Emerging Flux

Yuhao Chen, Jialiang Hu, Guanchong Cheng +4

New emerging flux (NEF) has long been considered a mechanism for solar eruptions, but detailed process remains an open question. In this work, we explore how NEF drives a coronal m…