Fig. 1
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Intensity map in Stokes I of all 47 observations. The mosaic is split into four parts for readability. Observations are taken from the western to eastern sides of the Sun. No merging images into a single mosaic using the overlap regions was attempted. To the upper right of each observation square is the μ value of each observation. All observations shown here come from the Stokes I observations of the Fe I 6301 Å line with a matched colour bar, with brighter colour showing more flux.
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