EGU23-17498, updated on 26 Feb 2023
https://doi.org/10.5194/egusphere-egu23-17498
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Internal gravity wave and tide interaction with geostrophic mean flow

Carsten Eden1, Pablo Sebastia Saez1, Manita Chouksey2, and Peter Dennert2
Carsten Eden et al.
  • 1Institut für Meereskunde, Universität Hamburg
  • 2Institut für Umweltphysik, Universität Bremen

Internal gravity waves (IGW) are ubiquitous in the open and coastal ocean. IGWs are refracted by their changing environment and may gain energy from or loose energy to the geostrophically balanced mean flow with vertical (wave drag) or horizontal shear (wave capture). Refraction, wave-wave interaction, or scattering at mean flow, topography, or turbulence can generate wave energy fluxes towards smaller wavelengths, where IGW break and mix density, which can drive in turn large scale mean flow. Two case studies of interaction of waves and mean-flow and their consequences for mixing are presented: Using a novel numerical model (IWEM) of the spectral energy balance of IGWs, we simulate the interaction of IGWs with an observed coherent meso-scale eddy in the coastal upwelling region off Mauretania. Using ray traycing we study the interaction of low mode IGWs at tidal frequencies (internal tides) with a geostrophic mean flow given by a realistic meso-scale eddy field.

How to cite: Eden, C., Sebastia Saez, P., Chouksey, M., and Dennert, P.: Internal gravity wave and tide interaction with geostrophic mean flow, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-17498, https://doi.org/10.5194/egusphere-egu23-17498, 2023.