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Multi-scale MHD approach to the current sheet filamentation in solar coronal reconnection

SYSNO ASEP	0352526
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Multi-scale MHD approach to the current sheet filamentation in solar coronal reconnection
Author(s)	Bárta, Miroslav (ASU-R)_{RID, ORCID} Büchner, J. (DE) Karlický, Marian (ASU-R)_{RID, ORCID}
Source Title	Advances in Space Research. - : Elsevier - ISSN 0273-1177 Roč. 45, č. 1 (2010), s. 10-17
Number of pages	18 s.
Language	eng - English
Country	GB - United Kingdom
Keywords	solar flares ; magnetic reconnection ; numerical MHD
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	GA205/07/1100 GA ČR - Czech Science Foundation (CSF)
	IAA300030701 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000273918100002
DOI	10.1016/j.asr.2009.07.025
Annotation	The main goal of the paper is to numerically investigate the relevance of cascading reconnection for solar flares. The numerical algorithm implemented for that purpose and first results are presented in this research note. Proposed algorithm – though motivated by the self-similar nature of MHD equations – belongs in fact to the class of block-structured Adaptive Mesh Refinement codes.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2011

Number of the records: 1