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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A visual transformer model trained on IRIS inversions predicts chromospheric temperature and density from SDO data with correlations around 0.8 on 80% of test cases.
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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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Predicting the thermodynamics in the chromosphere from the translation of SDO data into the IRIS$^{2}$ inversion results using a visual transformer model
A visual transformer model trained on IRIS inversions predicts chromospheric temperature and density from SDO data with correlations around 0.8 on 80% of test cases.