SST/CRISP observations of convective flows in a sunspot penumbra

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Fig. 12

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Radial variation of properties of spines and inter-spines, as defined by the LOS magnetic masks, shown in Fig. 6. The plots in the top row show field strengths and inclinations for spines (full) and inter-spines (dashed). Symbols in the lower four plots are as in Fig. 10.

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