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Infragravity-Frequency (0.005–0.05 Hz) Motions on the Shelf. Part I: Forced Waves

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1994

Year

TLDR

Infragravity‑frequency motions (0.005–0.05 Hz) on the continental shelf are investigated in this two‑part study. The study develops a bispectral technique to estimate forced and free infragravity wave energy and applies it in Part 2 to examine shelfwide variability of free infragravity energy. Using a 250 m × 250 m array of 24 bottom‑mounted pressure transducers at 13 m depth, the authors apply second‑order nonlinear theory and bispectral analysis to predict and quantify forced infragravity wave energy from surface gravity wave interactions. Predicted forced infragravity wave levels are generally lower than observed, indicating a mix of free and forced waves, with forced energy contributing up to ~30 % when infragravity energy peaks, and bispectral estimates confirm second‑order theory predictions.

Abstract

This is Part 1 of a two-part study of infragravity-frequency (nominally 0.005–0.05 Hz) motions on the continental shelf. Data from a large aperture (250 m × 250 m) array of 24 bottom-mounted pressure transducers deployed in 13 m depth is used to investigate the local forcing of infragravity motions by nonlinear difference-frequency interactions of surface gravity waves. Second-order nonlinear theory (Hasselmann) and observed swell-sea frequency-directional spectra are used to predict the energy levels of forced infragravity waves. For a wide range of wave conditions, the predicted forced wave levels are lower than the observed energy levels, suggesting that the infragravity band contains a mix of free and forced waves. Bispectral analysis is used to estimate the relative amounts of free and forced infragravity energy. Good agreement between bispectrum-based estimates and theoretical predictions of forced wave energy confirms that second-order nonlinear theory accurately predicts locally forced infragravity motions. The contribution of forced waves to the total infragravity energy, ranging from less than 0.1% to about 30%, is largest when the infragravity energy is maximum, consistent with previously noted trends in similar water depths. The bispectral technique developed here to estimate the energy of forced and free infragravity waves is used in Part 2 to investigate, with data from single-point pressure gauges, the shelfwide variability of free infragravity energy.