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This study presents an improved model for reconstructing the solar magnetic field over the past century by incorporating morphological asymmetry in sunspots. By using a Surface Flux Transport (SFT) model that accounts for the differences between leading and following sunspots, the researchers achieve better alignment with observational data, particularly in polar field development. The findings highlight the significance of morphological asymmetry in enhancing the accuracy of solar magnetic field simulation

Author

sezgiholmes

Language

EN