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

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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 on 2004 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 white-light, H alpha, extreme ultraviolet light, and soft and hard X-rays were also studied.

Metadaten
Author details:	Guan-Nan Gao, Min Wang, Jun Lin, Ning Wu, Cheng-Ming Tan, Bernhard Kliem ORCiD GND, Yang Su
DOI:	https://doi.org/10.1088/1674-4527/14/7/006
ISSN:	1674-4527
Title of parent work (English):	Research in astronomy and astrophysics : a publication of the Chinese Astronomical Society and National Astronomical Observatories, Chinese Academy of Sciences
Publisher:	Chinese Astronomical Society and National Astronomical Observatories, Chinese Academy of Sciences
Place of publishing:	Beijing
Publication type:	Article
Language:	English
Year of first publication:	2014
Publication year:	2014
Release date:	2017/03/27
Tag:	Sun: coronal mass ejections (CMEs); Sun: flares; Sun: magnetic reconnection; Sun: solar radio bursts
Volume:	14
Issue:	7
Number of pages:	12
First page:	843
Last Page:	854
Funding institution:	National Basic Research Program of China (973 program) [2011CB811403, 2013CBA01503]; National Natural Science Foundation of China [11273055, 11173010, 11333007, 10978006, 11103044, 11273030]; CAS [KJCX2-EW-T07, XDB09040202]; DFG; European Community Framework Programme 7, High Energy Solar Physics Data in Europe (HESPE) [263086]; Key Laboratory of Solar Activity, National Astronomical Observatories, CAS; Chinese Academy of Sciences [2012T1J0017]
Organizational units:	Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer review:	Referiert