Fig. 2.
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Polarimetric loops observed by ALMA at 229 GHz on 2017 Apr. 11. The observations began at T0= 9:20 UT (MJD 57854.39), 30 min after the peak of the X-ray flare. We highlight the small inner loop Atiny. Following the full loop Abig between T0 and T5, a similar pattern continues between T5 and T7, with a decreased period and reduced LP.
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