Fig. A.15

Jet 17: 2013 May 4 – Left panel: AIA 171 Å image of the jet, observed on 2013 May 4. The jet appeared to evolve from the edge of the active region, 11734 (S19 W04). The jet was associated with a closed loop structure and a complex, multi-threaded jet was originated from one of the footpoints of loop. It has been observed that the jet plasma couldn’t escape fully in the solar atmosphere, a part of it flows along the closed loop structure. The jet started its activity at 23:15 UT and lasted until 23:49 UT. Middle panel and right panel: the LOS HMI magnetogram image at 22:29 UT, before the jet evolution, and at 23:17 UT, during the jet evolution, respectively. The negative-polarity cancellation at nearby positive-polarity region was observed and is shown by white arrows. This magnetic activity lasted for a few hours and was co-temporal and co-spatial with the jet activity.
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