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

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    0352526 - ASÚ 2011 RIV GB eng J - Journal Article
    Bárta, Miroslav - Büchner, J. - Karlický, Marian
    Multi-scale MHD approach to the current sheet filamentation in solar coronal reconnection.
    Advances in Space Research. Roč. 45, č. 1 (2010), s. 10-17. ISSN 0273-1177. E-ISSN 1879-1948
    R&D Projects: GA ČR GA205/07/1100; GA AV ČR IAA300030701
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : solar flares * magnetic reconnection * numerical MHD
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 1.076, year: 2010

    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.
    Permanent Link: http://hdl.handle.net/11104/0192016

     
     
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