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Dynamics of Subsurface Flows in Solar Active Regions during the 2024 May Storm

In 2024 May, the Sun exhibited intense magnetic activity, marked by numerous high-intensity flares resulting from the interaction and merging of NOAA active regions (ARs) 13664 and 13668 in the southern hemisphere and AR 13663 in the northern hemisphere. Notably, AR 13664 displayed an extended lifet...

Ful tanımlama

Kaydedildi:
Asıl Yazarlar: B. Lekshmi, Sushanta Tripathy, Kiran Jain, Alexei Pevtsov
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2025-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Solar storm
Solar flares
Solar active region velocity fields
Solar active region magnetic fields
Solar active regions
Solar activity
Online Erişim:https://doi.org/10.3847/1538-4357/ade2e3
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