EGU26-8180, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-8180
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Monday, 04 May, 16:20–16:30 (CEST)
 
Room 0.31/32
Ocean Dynamics in Kilometre-Scale ICON Simulations
Nils Brüggemann1,2,3, Moritz Epke2, Helmuth Haak2, Peter Korn2, and Leonidas Linardakis2
Nils Brüggemann et al.
  • 1Leibniz Centre for Tropical Marine Research, Bremen, Germany (nils.brueggemann@mpimet.mpg.de)
  • 2Max Planck Institute for Meteorology
  • 3University of Bremen

We present the rich and versatile ocean dynamics emerging from a novel set of ICON ocean simulations with grid spacings around and below 1 km. 
Such configurations not only permit the explicit formation of submesoscale eddies but also enable a substantially richer representation of internal wave dynamics. 
We discuss the implications of these newly resolved processes for tracer transport, both by the explicitly resolved flow and through parameterized mixing processes. 
In particular, we demonstrate that submesoscale overturning along ocean fronts is explicitly resolved in these simulations. 
We further show how this overturning modifies density stratification and thereby interacts with small-scale turbulent processes. 
In addition, we demonstrate that the resolved portion of the internal wave spectrum is substantially extended at this resolution. 
Finally, we present first results illustrating how the improved representation of physical processes affects marine biogeochemistry. 
We conclude with an outlook on how these advances can improve the simulation of tropical upwelling systems in this new generation of ocean model configurations.

How to cite: Brüggemann, N., Epke, M., Haak, H., Korn, P., and Linardakis, L.: Ocean Dynamics in Kilometre-Scale ICON Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8180, https://doi.org/10.5194/egusphere-egu26-8180, 2026.