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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…
astro-ph.SR2025
A Wide-band High-frequency Type-II Solar Radio Burst
V. Vasanth, Yao Chen, G. Michalek
Type-II radio bursts are typically observed below ~ 400 MHz, with narrow-band slowly-drifting fundamental and harmonic structures. Here we report an unusual high-frequency wide-ban…