Radio observations of the fine structure inside a post-CME current sheet

A solar radio burst was observed in a coronal mass ejection/flare event by the Solar Broadband Radio Spectrometer at the Huairou Solar Observing Station on2004 December 1. The data exhibited various patterns of plasma motions, suggestive of the interaction between sunward moving plasmoids and the fl...

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Bibliographic Details
Published in:Research in astronomy and astrophysics 2014-07, Vol.14 (7), p.843-854
Main Authors: Gao, Guan-Nan, Wang, Min, Lin, Jun, Wu, Ning, Tan, Cheng-Ming, Kliem, Berhard, Su, Yang
Format: Article
Language:English
Subjects:
Astronomy
CME
Coronal mass ejection
Current sheets
Fine structure
Flares
Radio
Solar radio bursts
Stations
太阳观测站
射电爆发
射电观测
工作表
日冕物质抛射
等离子体团
精细结构
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Summary:A solar radio burst was observed in a coronal mass ejection/flare event by the Solar Broadband Radio Spectrometer at the Huairou Solar Observing Station on2004 December 1. The data exhibited various patterns of plasma motions, suggestive of the interaction between sunward moving plasmoids and the flare loop system during the impulsive phase of the event. In addition to the radio data, the associated whitelight, Hα, extreme ultraviolet light, and soft and hard X-rays were also studied.
ISSN:1674-4527
2397-6209
DOI:10.1088/1674-4527/14/7/006