collaborators

5 papers

astro-ph.SR2026

Three-dimensional evolution of a solar filament with multipoint observations

Qingmin Zhang, Jun Dai, Beili Ying +6

In this paper, we first devise a geometrical model, featuring a torus-like flux rope based on the shape of 3DCORE model. The global shape of the torus is an ellipse, while the cros…

astro-ph.SR2026

Magnetic Evolution of Highly-Sheared Region in Active Region 13842 Producing Large X9.0 Flare

Yijun Hou, Ting Li, Shuhong Yang +8

Shearing motion and magnetic flux cancellation around the polarity inversion line (PIL) play significant roles in the build-up of free magnetic energy and magnetic flux rope (MFR)…

astro-ph.SR2026

Can We Distinguish the Source Region Location of Filament/Prominence Eruptions from the Sun-as-a-star H Spectrum?

Junyi Zhang, Yijun Hou, Xiaofeng Liu +7

Solar filament/prominence eruptions can significantly perturb geospace when originating from favorable source locations and directions. While stellar analogs have been recently rep…

astro-ph.SR2026

The fine dynamics in homologous and recurrent jets induced by persistent rising loops and mini-filaments

Hengyuan Wei, Zhenghua Huang, Yadan Duan +1

Jets are common eruptive phenomena in the solar atmosphere which may occur repeatedly. Many studies of their fine dynamics have been conducted. However, the fine dynamics of persis…

astro-ph.SR2024

The magnetic origin of the mystery of rare H Moreton waves

Ze Zhong, Yao Chen, Y. W. Ni +4

Over the past three decades, a lot of coronal fast-mode waves were detected by space missions, but their counterparts in the chromosphere, called the Moreton waves, were rarely cap…