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One of the major unsolved problems in Solar Physics is that of CMEinitiation. In this paper, we have studied the initiation of a flare associatedCME which occurred on 2010 November 03 using multi-wavelength observationsrecorded by Atmospheric Imaging Assembly (AIA) on board Solar DynamicsObservatory (SDO) and Reuven Ramaty High Energy Solar Spectroscopic Imager(RHESSI). We report an observation of an inflow structure initially in304~{\AA} and in 1600~{\AA} images, a few seconds later. This inflow strucurewas detected as one of the legs of the CME. We also observed a non-thermalcompact source concurrent and near co-spatial with the brightening and movementof the inflow structure. The appearance of this compact non-thermal source,brightening and movement of the inflow structure and the subsequent outwardmovement of the CME structure in the corona led us to conclude that the CMEinitiation was caused by magnetic reconnection.

Initiation of CME event observed on November 3, 2010: Multi-wavelength Perspective