A Systematic Magnetic Polarity Inversion Line Data Set from SDO/HMI Magnetograms

A Systematic Magnetic Polarity Inversion Line Data Set from SDO/HMI Magnetograms

Magnetic polarity inversion lines (PILs) detected in solar active regions have long been recognized as arguably the most essential feature for triggering instabilities such as flares and eruptive events (i.e., eruptive flares and coronal mass ejections). In recent years, efforts have been focused on...

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Bibliographic Details
Main Authors: Anli Ji, Xumin Cai, Nigar Khasayeva, Manolis K. Georgoulis, Petrus C. Martens, Rafal A. Angryk, Berkay Aydin
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Astronomy software
Online Access:https://doi.org/10.3847/1538-4365/acb43a

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