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We observe a coronal jet around 22:08 UT on 23 rd March of 2017, in a quietregion towards the north-east of the solar disk. A minifilament eruption leadsto this jet. We analyze dynamics of the minifilament from its formation untilits eruption. We observe that the minifilament starts forming around 15:50 UT.Then at a later time, it disappears but again appears and finally erupts as ablowout jet around 22:08 UT. We study the evolution of photospheric magneticfield beneath the minifilament. Initially, we observe subsequent increase anddecrease of positive magnetic flux. Prior to the initiation of the eruption,positive magnetic flux shows a continuous decrease until the minifilamentdisappears. The positive magnetic flux increases and decreases due to newpositive flux emergence and cancellation of positive magnetic flux withnegative magnetic flux respectively.

Quiet Region Jet by Eruption of Minifilament and Associated Change in Magnetic Flux