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Radio Evidence of Break-out Reconnection?

SYSNO ASEP	0360869
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Radio Evidence of Break-out Reconnection?
Author(s)	Aurass, H. (DE) Mann, G. (DE) Zlobec, P. (IT) Karlický, Marian (ASU-R)_{RID, ORCID}
Source Title	Astrophysical Journal - ISSN 0004-637X Roč. 730, č. 1 (2011), 57/1-57/9
Number of pages	9 s.
Language	eng - English
Country	US - United States
Keywords	solarcorona ; coronal mass ejections ; solar flares
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000288453600056
DOI	10.1088/0004-637X/730/1/57
Annotation	We reconsider the 2003 October 28 X17 flare/coronal mass ejection (CME), studying the five minutes immediately before the impulsive flare phase (not discussed in previous work). To this aim we examine complementary dynamic radio spectrograms, single frequency polarimeter records, radio images, space-based longitudinal field magnetograms, and ultraviolet images. We find widely distributed faint and narrowband meter wave radio sources located outside active regions but associated with the boundaries of magnetic flux connectivity cells, inferred from the potential extrapolation of the observed photospheric longitudinal field as a model for coronal magnetic field structures.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2012

Number of the records: 1