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X-Ray Sources and Magnetic Reconnection in AN X-Class Flare

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    0031824 - ASÚ 2006 RIV NL eng C - Conference Paper (international conference)
    Veronig, A. - Vršnak, B. - Karlický, Marian - Temmer, M. - Magdalenic, J. - Dennis, B. R. - Otruba, W. - Pötzi, W.
    X-Ray Sources and Magnetic Reconnection in AN X-Class Flare.
    [Rentgenové zdroje a magnetická rekonexe v erupci typu X.]
    The Dynamic Sun: Challenges for Theory and Observations. Proceedings of the 11th European Solar Physics Meeting. Nizozemí: ESA Publications Division, 2005 - (Danesy, D.), ---. SP, 600. ISBN 92-9092-911-1.
    [European Solar Physics Meeting /11/. Leuven (BE), 11.09.2005-16.09.2005]
    R&D Projects: GA AV ČR IAA3003202; GA ČR GA205/04/0358
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : solar flares * X-ray emission * magnetic reconnection
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    RHESSI spectra indicate that during the time of loop-top source altitude decrease the emission of this source is generated by thermal bremsstrahlung from a superhot plasma with temperatures of 40 MK.

    RHESSI spektra ukazují, že během výškového poklesu rentgenového zdroje ve vrcholu magnetické smyčky je rentgenové záření generováno brzdným mechanizmem záření z plazmatu o teplotě 40 MK.
    Permanent Link: http://hdl.handle.net/11104/0132468

     
     
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