  The recent launch of the High resolution Coronal imager (Hi-C) provided a
unique opportunity to study the EUV corona with unprecedented spatial
resolution. We utilize these observations to investigate the properties of low
frequency (50-200 s) active region transverse waves, whose omnipresence had
been suggested previously. The five-fold improvement in spatial resolution over
SDO/AIA reveals coronal loops with widths 150-310 km and that these loops
support transverse waves with displacement amplitudes <50 km. However, the
results suggest that wave activity in the coronal loops is of low energy, with
typical velocity amplitudes <3 km/s. An extended time-series of SDO data
suggest low-energy wave behaviour is typical of the coronal structures both
before and after the Hi-C observations.
