Improved Reconstruction of the Century-long Solar Magnetic Field by Incorporating Morphological Asymmetry in Sunspots

Accurately modeling the solar magnetic field is important for understanding long-term solar activity and space weather, but it is challenging due to limited observations, especially near the Sun’s poles. The surface flux transport (SFT) model simulates how magnetic flux moves across the solar surfac...

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Bibliografische Detailangaben

Hauptverfasser:	Subhadip Pal, Gopal Hazra, Sudip Mandal
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	IOP Publishing 2026-01-01
Schriftenreihe:	The Astrophysical Journal
Schlagworte:	Sunspots Solar photosphere Solar magnetic fields Magnetohydrodynamical simulations Sunspot cycle
Online-Zugang:	https://doi.org/10.3847/1538-4357/ae5930
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