Recurrent Coronal Jets Induced by Repetitively Accumulated Electric Currents
Y. Guo, P. D\'emoulin, B. Schmieder, M. D. Ding, S. Vargas, Dom\'inguez, Y. Liu

TL;DR
This study links recurrent solar EUV jets to the buildup and release of electric currents caused by diverging photospheric flows, highlighting the role of magnetic reconnection in jet formation.
Contribution
First observation of rapid, cyclic electric current evolution associated with recurrent coronal jets using high-cadence magnetic data.
Findings
Electric currents peak in phase with EUV flux.
Current build-up and decay each last about 10 minutes.
Magnetic reconnection occurs periodically between bipoles and active region field.
Abstract
Three extreme-ultraviolet (EUV) jets recurred in about one hour on 2010 September 17 in the following magnetic polarity of active region 11106. The EUV jets were observed by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO). The Helioseismic and Magnetic Imager (HMI) on board SDO measured the vector magnetic field, from which we derive the magnetic flux evolution, the photospheric velocity field, and the vertical electric current evolution. The magnetic configuration before the jets is derived by the nonlinear force-free field (NLFFF) extrapolation. We derive that the jets are above a pair of parasitic magnetic bipoles which are continuously driven by photospheric diverging flows. The interaction drove the build up of electric currents that we indeed observed as elongated patterns at the photospheric level. For the first time, the high temporal…
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