  We present here the kinematics of the EUV wave associated with a GOES
M1.0-class solar flare, which originates in NOAA AR 12740. The event is
thoroughly observed with Atmospheric Imaging Assembly (AIA) onboard Solar
Dynamics Observatory (SDO) with high spatio-temporal resolutions. This event
displays many features of EUV waves, which are very decisive for the
understanding of the nature of EUV waves. These features include: a fast-mode
wave, a pseudo wave, a slow-mode wave and stationary fronts, probably due to
mode conversion. One fast-mode wave also propagates towards the coronal hole
situated close to the north pole and the wave speed does not change when it
encounters the coronal hole. We intend to provide self-consistent
interpretations for all these different features.
