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NLTE modelling of the flaring atmosphere above sunspot

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    0322314 - ASÚ 2009 RIV FR eng J - Journal Article
    Berlicki, A. - Heinzel, Petr - Schmieder, B. - Li, H.
    NLTE modelling of the flaring atmosphere above sunspot.
    [NLTE modelování erupční atmosféry nad skvrnami.]
    Astronomy & Astrophysics. Roč. 490, č. 1 (2008), s. 315-324. ISSN 0004-6361. E-ISSN 1432-0746
    Grant - others:EU(XE) ESA-PECS project No. 98030
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : Sun * flares * atmosphere
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 4.153, year: 2008

    New model of flares above sunspot penumbra was proposed. It was suggested that the observed flare emission results from flare loops overlaying the penumbra, rather than from the penumbral atmosphere itself. This model is consistent with multiwavelength spectral observations.

    Byl navržen nový model erupcí nad sluneční penumbrou. Bylo ukázáno, že pozorovaná emise ve spektrálních čarách pochází z erupčních smyček nad skvrnou a nikoliv z atmosféry penumbry. Tento model je konzistentní s multispektrálními pozorováními.
    Permanent Link: http://hdl.handle.net/11104/0170618

     
     
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