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Diapycnal mixing is crucial for ocean heat and carbon storage. Recent research focuses on its spatial variability, driven by internal waves, and develops new models for ocean dynamics.

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Area of Science:

  • Oceanography
  • Climate Science
  • Fluid Dynamics

Background:

  • Diapycnal mixing significantly impacts ocean thermodynamics, heat, and carbon cycles.
  • Observed mixing rates align with models, but spatial variability is substantial.
  • Internal waves are key drivers of turbulent mixing away from ocean boundaries.

Purpose of the Study:

  • To review progress in understanding internal-wave driven turbulent mixing.
  • To present dynamics-based parameterizations for global ocean models.
  • To explore mixing processes near internal tide generation, in the upper ocean, and at ocean margins.

Main Methods:

  • Developing and testing dynamics-based parameterizations for turbulent mixing.
  • Focusing on internal wave generation, propagation, and dissipation.
  • Implementing parameterizations in global ocean models.

Main Results:

  • Significant spatial variability in mixing rates across different ocean regions.
  • Tools developed for parameterizing internal-wave driven mixing.
  • Progress in modeling turbulence related to internal tides, near-inertial motions, and lee waves.

Conclusions:

  • Internal waves are a primary driver of ocean mixing.
  • Dynamics-based parameterizations improve representation of mixing in ocean models.
  • Further research is needed to refine models and understand mixing at ocean margins.