Atmospheric gravity waves (GWs) are small-scale wave disturbances that propagate in a three-dimensional (3D) manner from their sources; examples include flow over mountains, convection, fronts, and dynamically imbalanced flow systems (Fritts & Alexander, 2003). In the troposphere, their horizontal propagation is often visualized as stripe clouds aligned perpendicular to flows blowing over mountains. Although this mode is invisible, these waves also propagate vertically and play crucial roles in the dynamics and energy budget of the Earth's stratosphere, mesosphere, and lower thermosphere. Their propagation is strongly influenced by the background environment, especially horizontal and vertical shears in winds and static stability, as described by the GW ray-tracing equation (e.g., Marks & Eckermann, 1995).Changes in the stratospheric circulation associated with sudden stratospheric warming (SSW) events, such as deformation, displacement, breakup, and temporary disappearance of the stratospheric polar vortex, cause substantial changes in the propagation environment of GWs. Limpasuvan et al. (2011) performed mesoscale simulations of GWs during the 2008-2009 SSW and revealed a dominance of westward-propagating orographic GWs along the edge of the polar vortex prior to the SSW, which was greatly reduced after the occurrence of the SSW. During the SSW, they found westward-and eastward-propagating GWs in the polar region and attributed their possible generation mechanisms to a flow adjustment process in the stratosphere or secondary GW breaking. Their mesoscale model had a horizontal resolution of 10 km and a vertical resolution of 400 m. The simulation