ASR: Archival Solar Flares Catalog

Solar flares result from the rapid conversion of stored magnetic energy within the Sun’s corona. These energy releases are associated with coronal magnetic loops, which are rooted in dense photospheric plasma and are passively transported by surface advection. Their emissions cover a wide range of w...

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Bibliographic Details
Main Authors: M. Berretti, S. Mestici, L. Giovannelli, D. Del Moro, M. Stangalini, F. Giannattasio, F. Berrilli
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Online Access:https://doi.org/10.3847/1538-4365/adc731
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