  We study the recurring jets near AR11176 during the period 2011 March 31
17:00 UT to April 1 05:00 UT using observations from the Atmospheric Imaging
Assembly (AIA) on board Solar Dynamics Observatory (SDO). Mini-filaments
(mini-filament1 & 2) are found at the base of these recurring jets where
mini-filament1 shows the partial signature of eruption in case of Jet1-3.
However, the mini-filament2 shows a complete eruption driving a full blow-out
jet (Jet4). The eruption of mini-filament2 triggers C-class flare and Jet4
eruption. The eruption of Jet4 triggers a coronal mass ejection (CME). The
plane-of-sky velocity of recurring jets (Jet1-4) results in 160 km/s, 106 km/s,
151 km/s and 369 km/s. The estimated velocity of CME is 636 km/s. The
continuous magnetic flux cancellation is observed at the base of the jet
productive region which could be the cause of the eruption of mini-filaments
and recurring jets. In the former case, the mini-filament1 shows partial
eruption and first three jets (Jet1-3) are produced, but the rate of
cancellation was rather low. However, in the latter case, mini-filament2 fully
erupts (perhaps because of a higher cancellation rate), and this triggers a
C-class flare and a CME-productive jet. At the base of first three jets
(Jet1-3), the mini-filament1 causes to push the overlying dynamic complex thin
loops resulting in the reconnection and drives the jet (Jet1-3) eruptions. The
formation of the plasma blobs are observed during the eruption of the first jet
(Jet1).
