About my research

Near-Inertial Wave Dynamics

I am interested in the dynamics of near-inertial waves (NIWs) with a focus on understanding how their evolution is influenced by ocean turbulence. Near-inertial waves are ubiquitous in the ocean. They are forced by passing atmospheric storms and have a frequency close to the local Coriolis frequency. Despite NIWs often being regarded as a contaminant in observations, they exhibit rich dynamics that influence the climate system. Perhaps their most important role is in upper ocean mixing. Through a strong vertical shear, NIWs can induce mixing and deepening of the surface mixed layer. The dynamics of NIWs may be strongly modulated by the mesoscale eddy field. My thesis has focused on understanding this interaction in observations. I have used theoretical models of the NIW-mesoscale interactions to understand observations and quantify the role of various physical processes in the observed evolution of NIWs. I have also worked on understanding how the signature of NIW-mesoscale interactions may vary spatially in the ocean and how this may explain variations in the observed impact of the mesoscale eddy field on NIW evolution. The remainder of my thesis will try to extend theory of NIW-turbulence interactions to include submesoscale features as well as trying to observe this interaction in observations.

This animation shows simulations of the NIW-mesoscale interaction. The surface shows the mesoscale vorticity and the depth shows the wave activity (for NIWs this is proportional to the wave kinetic energy). There is rapid concentration of NIWs into anticyclones where they can propagate to depth.

Southern Ocean Dynamics

I also work on Southern Ocean dynamics with a focus on the Ross Sea. Bordering Antarctica in the Pacific sector, the Ross Sea is a fascinating region where problems in physical oceanography are strongly tied to problems in the dynamics of the atmosphere and cryosphere. Processes in the Ross Sea impact heat transfer to the Antarctic continental shelf with implications for ice melt. The Ross Sea also plays a role in the Southern Ocean's carbon cycle and in the meridional overturning circulation. In a warming climate, changes in the Ross Sea will both interact with and modulate changes in sea-ice, the Antarctic ice sheet and the local ecology. My research aims to understand the physical mechanisms governing the variability of the Ross Gyre. The Ross Gyre is a cyclonic, basin-scale circulation pattern that forms in the Ross Sea. Varability in the size and strength of the gyre has been shown to modulate the magnitude and pathways of heat transport from the open Southern Ocean towards Antarctica. I have been using idealised channel models of the Ross Sea to attempt to understand the physical drivers of variability in the Ross Gyre. These simulations have shown an important role for internal ocean variability and a connection between gyre variability and the Antarctic Circumpolar Current. By better understanding the mechanisms of gyre variability, we can better understand how the gyre may respond under climate change.

This animation shows idealised simulations of the Ross gyre. The colour maps represent the buoyancy in the model. The idealised bathymetry of the Ross gyre is shown in grey. We see tilting isopycnals associated with the ACC in the north of the domain. South of the zonal ridge, the isopycnals flatten. This is a signuature of the Ross gyre. Eddies can enter the gyre through its eastern boundary; at the end of the zonal ridge.