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 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
Verfasserangaben:	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
Titel des übergeordneten Werks (Englisch):	Research in astronomy and astrophysics : a publication of the Chinese Astronomical Society and National Astronomical Observatories, Chinese Academy of Sciences
Verlag:	Chinese Astronomical Society and National Astronomical Observatories, Chinese Academy of Sciences
Verlagsort:	Beijing
Publikationstyp:	Wissenschaftlicher Artikel
Sprache:	Englisch
Jahr der Erstveröffentlichung:	2014
Erscheinungsjahr:	2014
Datum der Freischaltung:	27.03.2017
Freies Schlagwort / Tag:	Sun: coronal mass ejections (CMEs); Sun: flares; Sun: magnetic reconnection; Sun: solar radio bursts
Band:	14
Ausgabe:	7
Seitenanzahl:	12
Erste Seite:	843
Letzte Seite:	854
Fördernde 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]
Organisationseinheiten:	Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer Review:	Referiert