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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Detaylı Bibliyografya
Asıl Yazarlar:	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
Materyal Türü:	Artigo
Dil:	Inglês
Baskı/Yayın Bilgisi:	EDP Sciences 2026-02-01
Seri Bilgileri:	Astronomy & Astrophysics
Konular:	sun: activity sun: corona sun: flares sun: particle emission sun: radio radiation
Online Erişim:	https://www.aanda.org/articles/aa/full_html/2026/02/aa55230-25/aa55230-25.html
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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

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