Fine-scale, weak opposite-polarity magnetic patches, likely low-lying loops, are found beneath the photospheric canopy of a solar plage and persist for tens of minutes.
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Fine-scale opposite-polarity magnetic fields in a solar plage revealed by integral field spectropolarimetry
Fine-scale, weak opposite-polarity magnetic patches, likely low-lying loops, are found beneath the photospheric canopy of a solar plage and persist for tens of minutes.