Saturation of the internal tide over the inner continental shelf. Part II: Parameterization

Author:

Becherer Johannes1,Moum James N.2,Calantoni Joseph3,Colosi John A.4,Barth John A.2,Lerczak James A.2,McSweeney Jacqueline M.2,MacKinnon Jennifer A.5,Waterhouse Amy F.5

Affiliation:

1. College of Earth, Ocean, and Atmospheric Sciences (CEOAS), Oregon State University, Corvallis, Oregon USA, and Helmholtz-Zentrum Hereon, Institute of Coastal Research, Geesthacht, Germany

2. College of Earth, Ocean, and Atmospheric Sciences (CEOAS), Oregon State University, Corvallis, Oregon

3. Ocean Sciences Division, U.S. Naval Research Laboratory, Stennis Space Center, MS 39529, USA

4. Department of Oceanography, Naval Postgraduate School, Monterey Bay, California

5. Scripps Institution of Oceanography, University of California, San Diego, La Jolla, California

Abstract

AbstractHere, we develop a framework for understanding the observations presented in the accompanying paper (Part I) by Becherer et al. (2021). In this framework, the internal tide saturates as it shoals due to amplitude limitation with decreasing water depth (H). From this framework evolves estimates of averaged energetics of the internal tide; specifically, energy, 〈APE〉, energy flux, 〈FE〉, and energy flux divergence, xFE〉. Since we observe that 〈D〉 ≈ xFE〉, we also interpret our estimate of xFE〉 as 〈D〉. These estimates represent a parameterization of the energy in the internal tide as it saturates over the inner continental shelf. The parameterization depends solely on depth-mean stratification and bathymetry. A summary result is that the cross-shelf depth dependencies of 〈APE〉, 〈FE〉 and xFE〉 are analogous to those for shoaling surface gravity waves in the surf zone, suggesting that the inner shelf is the surf zone for the internal tide. A test of our simple parameterization against a range of data sets suggests that it is broadly applicable.

Publisher

American Meteorological Society

Subject

Oceanography

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