EGU24-10545, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-10545
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Direct observations of coupled ice-ocean interactions within a basal terrace beneath Thwaites Eastern Ice Shelf

Peter Washam1, Britney Schmidt1, Keith Nicholls2, Peter Davis2, Clare Eayrs3, Veronica Hegelein1, Justin Lawrence4, Matt Meister1, Enrica Quartini1, David Holland5, and Frances Bryson1
Peter Washam et al.
  • 1Cornell University, Center for Astrophysics & Planetary Science, Ithaca, United States of America (pw389@cornell.edu)
  • 2British Antarctic Survey, Cambridge, United Kingdom
  • 3Korean Polar Research Institute, Incheon, South Korea
  • 4Honeybee Robotics, Altadena, United States of America
  • 5Courant Institute of Mathematical Sciences, New York University, United States of America

At present, considerable uncertainty surrounds the details of how Earth’s ice sheets interact with the surrounding ocean. This inhibits the reliability of future sea level rise projections from ice sheet models and highlights a need to better constrain ice-ocean interactions with in situ observations. Here, we present detailed ice and ocean data from beneath Thwaites Eastern Ice Shelf, Antarctica, collected with the underwater vehicle Icefin as part of the ITGC MELT project. The observations are a subset of the full data set that focus on the ice-ocean interactions within one 4-m-tall and 200-m-wide terrace formation in the ice base. We present ocean conditions in the terrace from 18 hydrographic profiles that reached within 1 cm of the ice along the feature’s flat roof and 13 cm from its steep sidewall. The ocean observations depict highly stable near-ice ocean stratification within 1 m of the terrace roof that break down near its sidewall, allowing warmer and more saline water to contact the ice there. The ocean observations are combined with ice base elevations and scaled morphological melt patterns in the ice to understand the dominant mechanisms driving ice-ocean interactions within this feature. We then input these data into the three-equation melt parameterization to estimate spatial variability in melt rates within these topographic features. We test various parameterizations for ocean heat flux into the flat and sloped ice surfaces, and compare the results to melt rates sampled along a nearby terrace sidewall and roof with a phase sensitive radar. This work in progress aims to better understand how ocean conditions interact with ice slope on small scales to drive variable melting in warm, highly stratified environments, with hopes of refining existing parameterizations of this process. We expect regions beneath much of the ice shelves occupying West Antarctica to interact similarly with the underlying ocean to what we observe beneath Thwaites. Hence, our observations hold relevance for how ice sheet models parameterize ocean-driven melting in this type of melt-driven regime.

How to cite: Washam, P., Schmidt, B., Nicholls, K., Davis, P., Eayrs, C., Hegelein, V., Lawrence, J., Meister, M., Quartini, E., Holland, D., and Bryson, F.: Direct observations of coupled ice-ocean interactions within a basal terrace beneath Thwaites Eastern Ice Shelf, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10545, https://doi.org/10.5194/egusphere-egu24-10545, 2024.