Mathematical models and time-frequency heat maps for surface gravity waves generated by thin ships

TL;DR

This paper develops mathematical models and uses time-frequency heat maps to analyze surface gravity waves generated by thin ships, aiming to infer vessel properties from wave signals, supported by experimental towing tank data.

Contribution

It introduces a methodology to match simple pressure-based models with complex ship wave theories in the time-frequency domain, enhancing wave analysis techniques.

Findings

Two-pressure minimal model replicates key features of Michell's theory

Time-frequency heat maps reveal interference patterns in ship waves

Experimental data supports the theoretical models

Abstract

Recent research suggests that studying the time-frequency response of ship wave signals has potential to shed light on a range of applications, such as inferring the dynamical and geometric properties of a moving vessel based on the surface elevation data detected at a single point in space. We continue this line of research here with a study of mathematical models for thin ships using standard Wigley hulls and Wigley transom-stern hulls as examples. Mathematical models of varying sophistication are considered. These include basic minimal models which use applied pressure distributions as proxies for the ship hull. The more complicated models are Michell's thin ship theory and the Hogner model, both of which explicitly take into account the shape of the hull. We outline a methodology for carefully choosing the form and parameter values in the minimal models such that they reproduce the key features of the more complicated models in the time-frequency domain. For example, we find that a two-pressure model is capable of producing wave elevation signals that have a similar time-frequency profile as that for Michell's thin ship theory applied to the Wigley hull, including the crucially important features caused by interference between waves created at the bow and stern of the ship. One of the key tools in our analysis is the spectrogram, which is a heat-map visualisation in the time-frequency domain. Our work here extends the existing knowledge on the topic of spectrograms of ship waves. The theoretical results in this study are supported by experimental data collected in a towing tank at the Australian Maritime College using model versions of the standard Wigley hulls and Wigley transom-stern hulls.