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In this study, we present the investigation of eleven recurring solar jetsoriginated from two different sites (site 1 and site 2) close to each other (~11 Mm) in the NOAA active region (AR) 12035 during 15--16 April 2014. The jetswere observed by the Atmospheric Imaging Assembly (AIA) telescope onboard theSolar Dynamics Observatory (SDO) satellite. Two jets were observed by theAryabhatta Research Institute of Observational Sciences (ARIES), Nainital,India telescope in H-alpha. On 15 April flux emergence is important in site 1while on 16 April flux emergence and cancellation mechanisms are involved inboth sites. The jets of both sites have parallel trajectories and move to thesouth with a speed between 100 and 360 km/s. We observed some connectionbetween the two sites with some transfer of brightening. The jets of site 2occurred during the second day and have a tendency to move towards the jets ofsite 1 and merge with them. We conjecture that the slippage of the jets couldbe explained by the complex topology of the region with the presence of a fewlow-altitude null points and many quasi-separatrix layers (QSLs), which couldintersect with one another.

Slippage of Jets Explained by the Magnetic Topology of NOAA Active Region 12035