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3D Whole-Prominence Fine Structure Model as a Test Case for Verification and Development of Magnetic Field Inversion Techniques

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    0552736 - ASÚ 2022 RIV US eng C - Conference Paper (international conference)
    Gunár, Stanislav - Mackay, D. H. - Štěpán, Jiří - Heinzel, Petr - Trujillo Bueno, J.
    3D Whole-Prominence Fine Structure Model as a Test Case for Verification and Development of Magnetic Field Inversion Techniques.
    Solar Polarization Workshop 8. San Francisco: Astronomical Society of the Pacific, 2019 - (Belluzzi, I.), s. 159-163. ASP Conference Series, 526. ISBN 978-1-58381-939-5. E-ISSN 1050-3390.
    [Solar Polarization Workshop 8. Florence (IT), 12.09.2016-16.09.2016]
    R&D Projects: GA ČR(CZ) GA16-17586S; GA ČR(CZ) GA16-16861S
    EU Projects: European Commission(XE) 328138 - COMBINED MHD AND RT
    Institutional support: RVO:67985815
    Keywords : 3D model * magnetic field * plasma environment
    OECD category: Astronomy (including astrophysics,space science)

    We show the potential of a new 3D whole-prominence fine structure model to serve as a well-controlled yet complex environment for testing inversion techniques for the magnetic field inference. The realistic 3D magnetic field and plasma environment provided by the model can be used for the direct synthesis of spectro-polarimetric data. Such synthetic data can be analyzed by advanced inversion tools and their results compared with the known properties provided by the model.

    Permanent Link: http://hdl.handle.net/11104/0327851

     
     
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