Context : Despite intensive studies of kink oscillations of coronal loops in the last decade , a large scale statistically significant investigation of the oscillation parameters has not been made using data from the Solar Dynamics Observatory ( SDO ) .

Aims : We carry out a statistical study of kink oscillations using Extreme Ultra-Violet ( EUV ) imaging data from a previously compiled catalogue .

Methods : We analysed 58 kink oscillation events observed by the Atmospheric Imaging Assembly ( AIA ) onboard SDO during its first four years of operation ( 2010-2014 ) .
Parameters of the oscillations , including the initial apparent amplitude , period , length of the oscillating loop , and damping are studied for 120 individual loop oscillations .

Results : Analysis of the initial loop displacement and oscillation amplitude leads to the conclusion that the initial loop displacement prescribes the initial amplitude of oscillation in general .
The period is found to scale with the loop length , and a linear fit of the data cloud gives a kink speed of C _ { k } = ( 1330 \pm 50 ) km s ^ { -1 } .
The main body of the data corresponds to kink speeds in the range C _ { k } = ( 800-3300 ) km s ^ { -1 } .
Measurements of 52 exponential damping times were made , and it was noted that at least 22 of the damping profiles may be better approximated by a combination of non-exponential and exponential profiles , rather than a purely exponential damping envelope .
There are an additional 10 cases where the profile appears to be purely non-exponential , and no damping time was measured .
A scaling of the exponential damping time with the period is found , following the previously established linear scaling between these two parameters .

Conclusions :