We present and discuss multi-wavelength observations of five homologous recurrent solar jets that occurred in active region NOAA 11133 on 11 December , 2010 .
These jets were well observed by the Solar Dynamic observatory ( SDO ) with high spatial and temporal resolution .
The speed of the jets ranged between 86 and 267 km s ^ { -1 } .
A type III radio burst was observed in association with all the five jets .
The investigation of the over all evolution of magnetic field in the source regions suggested that the flux was continuously emerging on longer term .
However , all the jets but J5 were triggered during a local dip in the magnetic flux , suggesting the launch of the jets during localised submergence of magnetic flux .
Additionally , using the PFSS modelling of the photospheric magnetic field , we found that all the jets were ejected in the direction of open field lines .
We also traced sunspot oscillations from the sunspot interior to foot-point of jets and found presence of \sim 3 minute oscillations in all the SDO/AIA passbands .
The wavelet analysis revealed an increase in amplitude of the oscillations just before the trigger of the jets , that decreased after the jets were triggered .
The observations of increased amplitude of the oscillation and its subsequent decrease provides evidence of wave-induced reconnection triggering the jets .