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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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SYSNO ASEP 0552736 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title 3D Whole-Prominence Fine Structure Model as a Test Case for Verification and Development of Magnetic Field Inversion Techniques Author(s) Gunár, Stanislav (ASU-R) RID, ORCID
Mackay, D. H. (GB)
Štěpán, Jiří (ASU-R) RID, ORCID
Heinzel, Petr (ASU-R) RID, ORCID
Trujillo Bueno, J. (ES)Source Title Solar Polarization Workshop 8. - San Francisco : Astronomical Society of the Pacific, 2019 / Belluzzi I. - ISBN 978-1-58381-939-5 Pages s. 159-163 Number of pages 5 s. Publication form Online - E Action Solar Polarization Workshop 8 Event date 12.09.2016 - 16.09.2016 VEvent location Florence Country IT - Italy Event type WRD Language eng - English Country US - United States Keywords 3D model ; magnetic field ; plasma environment Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) R&D Projects GA16-17586S GA ČR - Czech Science Foundation (CSF) GA16-16861S GA ČR - Czech Science Foundation (CSF) Institutional support ASU-R - RVO:67985815 Annotation 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.
Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2022
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