Abstract
The processes leading to the depletion of oceanic mesoscale kinetic energy (KE) and the energization of near-inertial internal waves are investigated using a suite of realistically forced regional ocean simulations. By carefully modifying the forcing fields we show that solutions where internal waves are forced have ∼ (Formula presented.) less mesoscale KE compared with solutions where they are not. We apply a coarse-graining method to quantify the KE fluxes across time scales and demonstrate that the decrease in mesoscale KE is associated with an internal wave-induced reduction of the inverse energy cascade and an enhancement of the forward energy cascade from sub-to super-inertial frequencies. The integrated KE forward transfer rate in the upper ocean is equivalent to half and a quarter of the regionally averaged near-inertial wind work in winter and summer, respectively, with the strongest fluxes localized at surface submesoscale fronts and filaments.
| Original language | English |
|---|---|
| Article number | e2021GL094376 |
| Journal | Geophysical Research Letters |
| Volume | 48 |
| Issue number | 18 |
| DOIs | |
| State | Published - 28 Sep 2021 |
| Externally published | Yes |
Keywords
- internal waves
- mesoscale eddies
- oceanic energy transfers
- submesoscale fronts
ASJC Scopus subject areas
- Geophysics
- General Earth and Planetary Sciences
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