  With the launch of SDO, many EUV waves were observed during solar eruptions.
However, the joint observations of Moreton and EUV waves are still relatively
rare. We present an event that a small-scale filament eruption simultaneously
results in a Moreton wave, an EUV wave and a Coronal Mass Ejection in active
region NOAA 12740. Firstly, we find that some dark elongate lanes or
filamentary structures in the photosphere existed under the small-scale
filament and drifted downward, which manifests that the small-scale filament
was emerging and lifting from subsurface. Secondly, combining the simultaneous
observations in different Extreme UltraViolet (EUV) and H$\alpha$ passbands, we
study the kinematic characteristics of the Moreton and EUV waves. The
comparable propagating velocities and the similar morphology of Moreton and
different passbands EUV wavefronts were obtained. We deduce that Moreton and
different passbands EUV waves were the perturbations in different
temperature-associated layers induced by the coronal magneto-hydrodynamic shock
wave. We also find the refracted, reflected and diffracted phenomena during the
propagation of the EUV wave. By using power-law fittings, the kinematic
characteristics of unaffected, refracted and diffracted waves were obtained.
The extrapolation field derived by the potential field source surface (PFSS)
model manifests that the existence of an interface of different magnetic system
(magnetic separatrix) result in refraction, reflection and deviation of the EUV
wave.
