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- W3160994923 abstract "A reduced-physics model is employed at 1/25° to 1/100° global resolution to determine (a) if linear dynamics can reproduce the observed low-mode M2 internal tide, (b) internal-tide sensitivity to bathymetry, stratification, surface tides, and dissipation parameterizations, and (c) the amount of power transferred to the nonstationary internal tide. The simulations predict 200 GW of mode-1 internal-tide generation, consistent with a general circulation model and semianalytical theory. Mode-1 energy is sensitive to damping, but a simulation using parameterizations for wave drag and wave-mean interaction predicts 84% of satellite observed sea-surface height amplitude variance on a 1° × 1° grid. The simulation energy balance indicates that 16% of stationary mode-1 energy is scattered to modes 2–4 and negligible energy propagates onto the shelves. The remaining 84% of energy is lost through parameterizations for high-mode scattering over rough topography (54%) and wave-mean interactions that transfer energy to the nonstationary internal tide (29%)." @default.
- W3160994923 created "2021-05-24" @default.
- W3160994923 creator A5001736264 @default.
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- W3160994923 date "2021-06-05" @default.
- W3160994923 modified "2023-10-10" @default.
- W3160994923 title "Global Dynamics of the Stationary M <sub>2</sub> Mode‐1 Internal Tide" @default.
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- W3160994923 doi "https://doi.org/10.1029/2020gl091692" @default.
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