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Fig. 6


LOS magnetic field component in the chromosphere versus the LOS magnetic field component in the photosphere for the He components with retrieved LOS velocity in the range −30 < vLOS <  −10 km s-1 (top left), 30 < vLOS < 110 km s-1 (top right), and − 10 < vLOS < 10 km s-1 (bottom panels). The green lines represent linear regressions.

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