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
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
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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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.