Fig. 13

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ROI from a five-second (500 frames) average of quiet Sun Stokes spectra from the 2017 SST/TRIPPLE-SP campaign. Panels in the upper row present data with no correction applied, while the middle row shows the same after spectroflat and our wavelength calibration are applied. The lower row panels show the same ROI, after the Wöhl et al. (2002) method is applied. Note: any instrumental cross-talk was not corrected in any of these datasets.
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