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Dynamics of quiescent prominence fine structures analyzed by 2D non-LTE modelling of the Hα line

  1. 1.
    SYSNO ASEP0386855
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleDynamics of quiescent prominence fine structures analyzed by 2D non-LTE modelling of the Hα line
    Author(s) Gunár, Stanislav (ASU-R) RID, ORCID
    Mein, P. (FR)
    Schmieder, B. (FR)
    Heinzel, Petr (ASU-R) RID, ORCID
    Mein, N. (FR)
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 543, July (2012), A93/1-A93/15
    Number of pages15 s.
    Languageeng - English
    CountryFR - France
    KeywordsSun ; filaments ; prominences
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGP205/09/P554 GA ČR - Czech Science Foundation (CSF)
    GAP209/12/0906 GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    UT WOS000306597200093
    DOI10.1051/0004-6361/201218940
    AnnotationThe combination of 2D non-LTE prominence fine-structure modelling with the statistical analysis of the observed and synthetic Lyman and Hα spectra allows us to analyze the influence of the model input parameters and the velocity fields on the synthetic Hα line profiles, thus determine the overall dynamics of the observed prominence as well as the physical parameters of its plasma.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2013
Number of the records: 1  

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