Fig. 5.
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Intensity (first column), Stokes Q (second column), U (third column), and V (fourth column) profiles, normalised to the average quiet-Sun continuum intensity, Ic. The top row shows the spectra in channel 1, which includes the Si I line at 10827 Å and the He I triplet at 10830 Å. The bottom row shows the spectra in channel 2, which includes most of the Ca II line at 8542 Å. The displayed profiles correspond to the pixel at (33, 57) arcsec, the orange square in Fig. 2, which is associated with a quiet-Sun area with low magnetic activity.
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