On the Differences in the Periodic Behavior of Magnetic Helicity Flux in Flaring Active Regions | Szabolcs Soós
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03.03.2022
Co-author
Affiliation
Eötvös Loránd University (ELTE), Hungary
Main category
Natural Sciences (Astrophysics and Astrononmy)
Caption
Observational precursors of large solar flares provide a basis for future operational systems for forecasting. We studied the evolution of the normalized emergence (EM), shearing (SH), and total (T) magnetic helicity flux components for 14 flaring (with at least one X-class flare) and 14 nonflaring (
Further information
Further reading
Link to the European Solar Physics Online Seminars (ESPOS) webpage: https://espos.stream/2022/03/03/Soos/
Language
English
DOI
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