Flare-associated type III radio bursts and dynamics of the EUV jet from SDO/AIA and RHESSI observations

Naihwa Chen, Wing Huen Ip, Davina Innes

研究成果: 雜誌貢獻期刊論文同行評審

20 引文 斯高帕斯(Scopus)

摘要

We present a detailed description of the interrelation between the Type III radio bursts and energetic phenomena associated with the flare activities in active region AR11158 at 07:58 UT on 2011 February 15. The timing of the Type III radio burst measured by the radio wave experiment on Wind/WAVE and an array of ground-based radio telescopes coincided with an extreme-ultraviolet (EUV) jet and hard X-ray (HXR) emission observed by SDO/AIA and RHESSI, respectively. There is clear evidence that the EUV jet shares the same source region as the HXR emission. The temperature of the jet, as determined by multiwavelength measurements by Atmospheric Imaging Assembly, suggests that Type III emission is associated with hot, 7 MK, plasma at the jet's footpoint.

原文???core.languages.en_GB???
文章編號96
期刊Astrophysical Journal
769
發行號2
DOIs
出版狀態已出版 - 1 6月 2013

指紋

深入研究「Flare-associated type III radio bursts and dynamics of the EUV jet from SDO/AIA and RHESSI observations」主題。共同形成了獨特的指紋。

引用此