What drives decayless kink oscillations in active-region coronal loops on the Sun?

Here, we present a study of the phenomena decayless kink oscillations in system active-region (AR) coronal loops. Using high-resolution observations from two different instruments, namely Extreme Ultraviolet Imager (EUI) on board Solar Orbiter and Atmospheric Imaging Assembly (AIA) Dynamics Observatory, follow these AR loops for an hour each three consecutive days. Our results show significantly more resolved waves higher resolution EUI data compared with AIA data. Furthermore, same exhibits many Day 2, while detect very few 3 , find none at all 1. Analysis photospheric magnetic field reveals that, most time, were rooted sunspots, where supergranular flows are generally absent. This suggests that flows, which often invoked as drivers waves, not necessarily driving such our observations. Similarly, findings also cast doubt other possible transient driver or mode conversion longitudinal near loop footpoints. In conclusion, analysis commonly suspected sources proposed to drive seem be operating this event, therefore search elusive wave needs continue.