EGU21-14207, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-14207
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Near-inertial waves modulated by background flow in realistic global ocean simulations

Keshav Raja1, Maarten Buijsman1, Oladeji Siyanbola1, Miguel Solano1, Jay Shriver2, and Brian Arbic3
Keshav Raja et al.
  • 1School of Ocean Science and Engineering, University of Southern Mississippi, Stennis Space Center, United States of America
  • 2Ocean Dynamics and Prediction Branch, Naval Research Laboratory, Stennis Space Center, United States of America
  • 3Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, Michigan, United States of America

Wind generated near-inertial waves (NIWs) are a major source of energy for deep-ocean mixing by transmitting wind energy from the ocean surface into the interior. Recently, it has been established that the NIW energy transmission to ocean depths is significantly modulated by background mesoscale vorticity. Thus, understanding NIW energetics in the presence of mesoscale eddies on a global scale is crucial.

We study the generation, propagation and dissipation of NIWs in global 1/25o Hybrid Coordinate Ocean Model (HYCOM) simulations with realistic tidal forcing. The model has 41 layers with uniform vertical coordinates in the mixed layer and isopycnal coordinates in the ocean interior. The model is forced by 1/3hr wind from the NAVGEM atmospheric model. We analyze one month of model data for May-June 2019. The 3D HYCOM fields are projected on vertical normal modes to compute the wind input, wave kinetic energy (KE), flux divergence and dissipation per mode.

We find that the globally integrated wind input in surface near-inertial motions is 0.21 TW for the 30-day period and is consistent with previous studies. The sum of the wind input to the first 5 modes accounts to only 31% of the total wind input while the sum of the NIW kinetic energy in the first 5 modes adds up to 60% of the total NIW KE. The difference in the fraction of the total between the wind input and NIW KE (31% and 60%) suggests that a significant portion of wind-induced near-inertial motions is dissipated close to the surface without being projected onto modes. We also find that NIW horizontal fluxes diverge from areas with cyclonic vorticity and converge in areas with anticyclonic vorticity, i.e., anticyclonic eddies are a sink for NIW energy in the global ocean.

The residual NIW KE that does not project onto modes is found to be largely trapped in anticyclonic eddies. In a next step, we will study the fate of this energy, which most likely propagate downward as beam-like features with large wave numbers. We will compute the near-inertial wave energy balance for fixed subsurface layers and consider the energy exchange between these layers to understand the vertical structure of NIW energy dissipation. We find that the downward NIW radiation to the ocean interior at 500 m depth is 19% of the surface near-inertial wind input for the 30-day period.

How to cite: Raja, K., Buijsman, M., Siyanbola, O., Solano, M., Shriver, J., and Arbic, B.: Near-inertial waves modulated by background flow in realistic global ocean simulations, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-14207, https://doi.org/10.5194/egusphere-egu21-14207, 2021.

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