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Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202038900
Abstract: Obtaining the magnetic field vector accurately in the solar atmosphere is essential for studying changes in field topology during flares and to reliably model space weather. We tackle this problem by applying various inversion methods…
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Keywords:
non lte;
field;
confined flare;
lte inversions ... See more keywords