A solar jet-induced perturbation propagating through coronal loops and in-loop electron beam transport as indicated by type II and type N radio bursts

Aims. 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 occur in the absence of a CME and to be associated with weak solar activity. The aim of this study is to identify...

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Detalhes bibliográficos

Principais autores:	Cui Yingli, Kong Xiangliang, Li Zhentong, Wang Bing, Duan Yadan, Zhong Ze, Ning Hao, Wu Zhao, Wang Manqing, Liu Yang, Yu Feiyu, Jiang Zelong, Chen Wei, Su Yang, Chen Yao
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-02-01
coleção:	Astronomy & Astrophysics
Assuntos:	sun: activity sun: corona sun: flares sun: particle emission sun: radio radiation
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/02/aa55230-25/aa55230-25.html
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