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Fig. 7


Zoomed-in view of the solar jet region where the positive (white) and negative (black) photospheric magnetic field can be seen as contours overlaid on the AIA 171 Å images. The contours are drawn at 150 G. The inset on the top left of each panel represents a zoomed-in view of the photospheric magnetic field from HMI in the dashed rectangular box. The positive polarity footpoint responsible for the jet activity is indicated by the white arrow in (c).

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