Fig. 1.
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Small-scale loop system known as a coronal bright point. Left to right: AIA 193 Å, IRIS SJI 1400, and HMI magnetogram images with the CBP in the centre of the field of view (FOV). The red and blue contours trace magnetic fluxes at ±50 G. The HMI magnetograms are saturated at ±50 G. The white-line square in the first panel outlines the FOV shown in Fig. 2.
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