  In this study, we present geometrical and kinematical analysis of Moreton
wave observed in 2012 June 3rd and July 6th, recorded in H-$\alpha$ images of
Global Oscillation Network Group (GONG) archive. These large-scale waves
exhibit different features compared to each other. The observed wave of June
3rd has angular span of about $70^{\circ}$ with a diffuse wave front associated
to NOAA active region 11496. It was found that the speed of the wave that
started propagating at 17.53 UT is about $931\pm80$ km/s. The broadness nature
of this Moreton wave can be interpreted as the vertical extension of the wave
over the chromosphere. On the other hand, the wave of July 6th may be
associated to X1.1 class flare that occurred at 23.01 UT around the 11515
active region. From the kinematical analysis, the wave propagated with the
initial velocity of about $994\pm70$ km/s which is in agreement with coronal
shock velocity derived from type II radio burst observation, $v\sim1100$ km/s.
These two identified waves add the inventory of the large-scale waves observed
in 24th Solar Cycle.
