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Response of optical hydrogen lines to beam heating. I. Electron beams

  1. 1.
    SYSNO ASEP0334858
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleResponse of optical hydrogen lines to beam heating. I. Electron beams
    TitleOdezva optických čar vodíku na ohřev svazky: 1. Elektronové svazky
    Author(s) Kašparová, Jana (ASU-R) RID, ORCID
    Varady, M. (CZ)
    Heinzel, Petr (ASU-R) RID, ORCID
    Karlický, Marian (ASU-R) RID, ORCID
    Moravec, Z. (CZ)
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 499, č. 3 (2009), s. 923-934
    Number of pages12 s.
    Languageeng - English
    CountryFR - France
    Keywordssolar flares ; radiative transfer ; hydrodynamics
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGA205/04/0358 GA ČR - Czech Science Foundation (CSF)
    GP205/06/P135 GA ČR - Czech Science Foundation (CSF)
    GA205/07/1100 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000266730600033
    DOI10.1051/0004-6361/200811559
    AnnotationWe investigate the role of non-thermal electrons in the formation regions of Hα, Hβ, and Hγ lines in order to unfold their influence on the formation of these lines. We concentrate on pulse-beam heating varying on a subsecond timescale. Furthermore, we theoretically explore possibility that a new diagnostic tool exists indicating the presence of non-thermal electrons in the flaring chromosphere based on observations of optical hydrogen lines.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2010
Number of the records: 1  

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