  We show that turbulence in core collapse supernovae (CCSNe) which has been
shown recently to ease shock revival might also lead to the formation of
intermittent thick accretion disks, or accretion belts, around the newly born
neutron star (NS). The accretion morphology is such that two low density
funnels are formed along the polar directions. The disks then are likely to
launch jets with a varying axis direction, i.e., jittering-jets, through the
two opposite funnels. The energy contribution of jets in this jittering jets
mechanism might result in an explosion energy of E>10^51erg, even without
reviving the stalled shock. We strengthen the jittering jets mechanism as a
possible explosion mechanism of CCSNe.
