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Fig. 12.

image

Anticlockwise motion of newly-emerged flux around the pre-existing positive (leading) sunspot in NOAA AR 11585. Tracked fragments of flux are labelled A–C. In each image, vectors are drawn either to connect the flux-weighted centroids of two orbiting fragments (panels a-c) or to best-fit the major axis of merged fragments (panels d-f). This figure is available as an online movie.

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