3 papers
astro-ph.SR2026
Observational Evidence of Solar Spicules Associated with Microfilament Eruptions Using DKIST
Qifan Dong, Xiaoli Yan, Zhike Xue +8
The formation mechanism of spicules is fundamentally important for understanding mass and energy transport from the chromosphere into the corona. Recent studies suggested that spic…
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.SR2025
Solar jet-induced perturbation propagating through coronal loops and in-loop electron beam transport indicated by type II and type N radio bursts
Yingli Cui, Xiangliang Kong, Zhentong Li +12
Solar type II radio bursts are commonly attributed to coronal shocks driven by coronal mass ejections (CMEs). However, some metric type II bursts have occasionally been reported to…