Gravity waves (GWs) are key drivers of the atmospheric general circulation. They transport a significant fraction of the momentum needed to constrain the atmospheric mean flow above the troposphere. GWs are generated by a complex mix of sources primarily located at surface and lower-atmospheric levels (e.g., Fritts & Alexander, 2003, and references therein). One of the most intense regions of GW activity is the stratosphere above the Southern Ocean in austral winter (e.g., Hindley et al., 2015, and references therein). Despite the known importance of GWs to the dynamics of this region, weather and climate models are known to consistently underestimate GW momentum fluxes here. This leads to significant biases in the simulated large-scale circulation (e.g., Garcia et al., 2017; McLandress et al., 2012). Therefore, understanding the sources and propagation characteristics of GWs is vitally important to improving our understanding and simulations of the Antarctic high-latitude circulation, which in turn impacts upon weather, ozone and climate processes at both local and global scales (e.g.,