At a broad scale, evolution of the oceanic lithosphere-asthenosphere system follows a relatively simple half-space cooling model with a rigid plate overlying weaker asthenosphere that thickens with distance from the ridge. However, in detail observations such as seafloor shallowing relative to half-space cooling at ages >70 Ma and seafloor gravity lineations suggest deviations from this simple model. One candidate to explain these observations is small-scale convection, which has been proposed in the form of so-called “Richter rolls”. These convective cells are estimated to be ~200 km in diameter and bring hot material toward the Earth’s surface.
The YoungORCA experiment
The YoungORCA project consists of an array of 30 broadband ocean-bottom seismometers (OBS) and aims to directly image small-scale convection. Located at ~40 Ma seafloor in the south Pacific, the array sits on distinct gravity undulations of ~200 km wavelength that may indicate convective cells in the current-day asthenosphere.
My research utilizes surface waves (Rayleigh and Love) to investigate the physical, chemical, and thermal structure of the uppermost mantle beneath the array. These waves range in sensitivity from the crust down to ~300 km depth in the uppermost asthenosphere. From surface-wave observations of phase velocity, we constrain the shear velocity structure in the upper mantle, as well as seismic anisotropy.
We find evidence for small-scale convection beneath the YoungORCA array. Seismic anisotropy in the asthensophere reveals a fast direction rotated significantly (~25º) from the absolute plate motion (APM) direction, at odds with the predicted large-scale mantle circulation pattern. This clockwise rotation in anisotropy relative to APM may be explained by pressure-drive flow associated with the South Pacific Superswell. As hot mantle material upwells and impinges on the lithosphere, mantle should flow radially away from the plume head, producing a secondary flow direction that is consistent with what we observe.