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Using high spatial and temporal data from the New Vacuum Solar Telescope(NVST) and the Solar Dynamics Observatory (SDO), we present unambiguousobservations of recurrent two-sided loop jets caused by magnetic reconnectionbetween erupting minifilaments and nearby large filament. The observationsdemonstrate that three two-sided loop jets, which ejected along the largefilament in opposite directions, had similar appearance and originated from thesame region. We find that a minifilament erupted and drove the first jet. Itreformed at the same neutral line later, and then underwent partial and totaleruptions, drove the second and third jets, respectively. In the course of thejets, cool plasma was injected into the large filament. Furthermore, persistentmagnetic flux cancelation occurred at the neutral line under the minifilamentbefore its eruption and continued until the end of the observation. We inferthat magnetic flux cancellation may account for building and then triggeringthe minifilament to erupt to produce the two-sided loop jets. This observationnot only indicates that two-sided loop jets can be driven by minifilamenteruptions, but also sheds new light on our understanding of the recurrentmechanism of two-sided loop jets.

Recurrent Two-Sided Loop Jets Caused by Magnetic Reconnection between Erupting Minifilaments and Nearby Large Filament