Active-region magnetic fields modulate deeper meridional flows in the Sun's near-surface shear layer, driving episodic poleward flux transport and hemispheric asymmetries in polar field evolution.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
fields
astro-ph.SR 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Observational report of polar polarity reversal times in solar cycle 25 from Hinode data, with northern reversal in November 2024 and southern in October 2024.
Long-term 17 GHz microwave polar brightening shows strong correlations with polar coronal hole area and polar magnetic field strength.
citing papers explorer
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Active-region Modulation of Subsurface Meridional Flows and Magnetic Flux Transport on the Sun
Active-region magnetic fields modulate deeper meridional flows in the Sun's near-surface shear layer, driving episodic poleward flux transport and hemispheric asymmetries in polar field evolution.
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Polarity Reversal of the Polar Magnetic Fields in Solar Cycle 25
Observational report of polar polarity reversal times in solar cycle 25 from Hinode data, with northern reversal in November 2024 and southern in October 2024.
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Microwave Polar Brightening and Its Connection to Polar Coronal Holes
Long-term 17 GHz microwave polar brightening shows strong correlations with polar coronal hole area and polar magnetic field strength.