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

0552736 - ASÚ 2022 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
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]
Grant CEP: GA ČR(CZ) GA16-17586S; GA ČR(CZ) GA16-16861S
GRANT EU: European Commission(XE) 328138 - COMBINED MHD AND RT
Institucionální podpora: RVO:67985815
Klíčová slova: 3D model * magnetic field * plasma environment
Obor OECD: 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.

Trvalý link: http://hdl.handle.net/11104/0327851