Investigation on the Formation of Herringbone Structure in TypeⅡSolar Radio Bursts  

作　　者：Z.Z.Abidin A.N.Zulkiplee V.Epin F.A.M.Pauzi 

机构地区：[1]Radio Cosmology Research Lab,Physics Dept.,Faculty of Science,University of Malaya,Kuala Lumpur,Malaysia

出　　处：《Research in Astronomy and Astrophysics》2023年第5期101-109,共9页天文和天体物理学研究（英文版）

基　　金：the Faculty of Science,University of Malaya(grant No.GPF081-2020)for their funding。

摘　　要：We report detailed observation of the“herringbone”of a Type II solar radio burst that occurred on 2010 November 3rd.Data from the Space Weather Prediction Center,National Oceanic and Atmospheric Administration,e-CALLISTO,and Nan?ay Radio Heliograph are analyzed.We determine the brightness temperature and degree of circular polarization of the“herringbone”burst.Correlations between the physical parameters and the“herringbone”are examined.Based on the relationship,this is the first study that suggested this“herringbone”was generated through fundamental plasma.

关 键 词：SUN activity-Sun corona-Sun coronal mass ejections(CMEs)-Sun magnetic fields-Sun radio radiation 

分 类 号：P182[天文地球—天文学]