  We present the observations of an extreme-ultraviolet (EUV) wave, which
originated from the active region (AR) NOAA 12887 on 28 October 2021 and its
impact on neighbouring loops. The event was observed by the Atmospheric Imaging
Assembly (AIA) on board the Solar Dynamics Observatory (SDO) satellite at
various wavebands and by the Solar TErrestrial RElations Observatory-Ahead
(STEREO-A) with its Extreme-Ultraviolet Imager (EUVI) and COR1 instruments with
a different view angle than SDO. We show that the EUV wave event consists of
several waves as well as non-wave phenomena. The wave components include: the
fast-mode part of the EUV wave event, creation of oscillations in nearby loops,
and the appearance of wave trains. The non-wave component consists of
stationary fronts. We analyze selected oscillating loops and find that the
periods of these oscillations range from 230 - 549 s. Further, we compute the
density ratio inside and outside the loops and the magnetic field strength. The
computed density ratio and magnetic field are found in the range of 1.08 - 2.92
and 5.75 - 8.79 G, respectively. Finally, by combining SDO and STEREO-A
observations, we find that the observed EUV wave component propagates ahead of
the CME leading edge.
