activity
20242026
collaborators

7 papers

astro-ph.HE2026

Twisted-pair unilateral reconnection: A unifying driver for magnetically powered astrophysical bursts

Shu-Ping Yan, Wenhui Yu, Jing Ye +11

Magnetic reconnection in twisted loops has long been invoked as an engine powering energetic transients from black hole accretion to neutron star mergers, yet never directly observ…

astro-ph.SR2025

The Solar Close Observations and Proximity Experiments (SCOPE) mission

Jun Lin, Jing Feng, Zhenhua Ge +31

The Solar Close Observations and Proximity Experiments (SCOPE) mission will send a spacecraft into the solar atmosphere at a low altitude of just 5 R_sun from the solar center. It…

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

The effect of plasma- on the heating mechanisms during magnetic reconnection in partially ionized low solar atmosphere

Abdullah Zafar, Lei Ni, Kaifeng Kang +5

We performed numerical simulations of magnetic reconnection with different strength of magnetic fields from the solar photosphere to the upper chromosphere. The main emphasis is to…

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…