Surprisingly low near-inertial energy flux leaving the ocean’s mixed layer
Abstract:
The previous studies on the subject indicate that a large portion of wind-power input to NI motions is dissipated in a surface layer of fixed depth and in specific regions in the ocean. In comparison, we study in detail the spatial and temporal variability of the ocean’s ML and gives an estimate on a global scale, which allows for the first time for a global quantification of the transfer of NI energy into the deep layers of the ocean. We address the following questions: What is the magnitude of the wind-power input to NI motions simulated with our high-resolution ocean model? How large is the fraction of the total wind-induced NI energy flux that leaves the ML? What are the main factors that control this fraction?
The wind-power input to surface NI motions amounts to 0.35 TW, of which a fraction of about 11% i.e., 0.04 TW leaves the ML and propagates into the stratified interior of the ocean. Locally, this fraction tends to decrease with increasing depth of the ML and with increasing strength of wind stress variability, indicating the strong control of the turbulent dissipation inside the ML on the fraction. The low power input by NI waves points towards the importance of other energy sources (like the dissipation of mesoscale eddy energy) for interior mixing to sustain the global general circulation in the ocean.
