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Physics > Atmospheric and Oceanic Physics

Title: The influence of vertical resolution on internal tide energetics and subsequent effects on underwater acoustic propagation

Abstract: Internal tide generation and breaking play a primary role in the vertical transport and mixing of heat and other properties in the ocean interior, thereby influencing climate regulation. Additionally, internal tides increase sound speed variability in the ocean, consequently impacting underwater acoustic propagation. With advancements in large-scale ocean modeling capabilities, it is essential to assess the impact of higher model resolutions (horizontal and vertical) in representing internal tides. This study investigates the influence of vertical resolution on internal tide energetics and its subsequent effects on underwater acoustic propagation in the HYbrid Coordinate Ocean Model (HYCOM). An idealized configuration with a ridge, forced only by semidiurnal tides and having 1-km horizontal grid-spacing, is used to test two different vertical-grid discretizations, defined based on the zero-crossings of horizontal velocity eigenfunctions, with seven distinct numbers of isopycnal layers, ranging from 8 to 128. Analyses reveal that increasing the number of layers up to 48 increases barotropic-to-baroclinic tidal conversion, available potential energy, and vertical kinetic energy, reaching equilibrium afterwards with higher layer counts. Vertical shear exhibits a similar pattern but converging at 96 layers. Simulations with at least 48 layers fully resolve the available potential energy contained in the 3rd to 8th tidal baroclinic modes. Finally, sound speed variability and acoustic parameters differ for simulations with less than 48 layers. Therefore, the study concludes that a minimum vertical resolution (48 layers in this case) is required in isopycnal models to minimize the impact on internal tide properties and associated underwater acoustic propagation.
Subjects: Atmospheric and Oceanic Physics (physics.ao-ph)
Cite as: arXiv:2404.05924 [physics.ao-ph]
  (or arXiv:2404.05924v1 [physics.ao-ph] for this version)

Submission history

From: Luna Hiron [view email]
[v1] Tue, 9 Apr 2024 01:04:26 GMT (1996kb)

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