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36 Integrals with Coalescing SaddlesApplications

§36.13 Kelvin’s Ship-Wave Pattern

A ship moving with constant speed V on deep water generates a surface gravity wave. In a reference frame where the ship is at rest we use polar coordinates r and \phi with \phi=0 in the direction of the velocity of the water relative to the ship. Then with g denoting the acceleration due to gravity, the wave height is approximately given by

where

36.13.2\rho=\ifrac{gr}{V^{2}}.

The integral is of the form of the real part of (36.12.1) with y=\phi, u=\theta, g=1, k=\rho, and

36.13.3f(\theta,\phi)=-\frac{\mathop{\cos\/}\nolimits\!\left(\theta+\phi\right)}{{%
\mathop{\cos\/}\nolimits^{{2}}}\theta}.

When \rho>1, that is, everywhere except close to the ship, the integrand oscillates rapidly. There are two stationary points, given by

36.13.4
\theta_{{+}}(\phi)=\tfrac{1}{2}(\mathop{\mathrm{arcsin}\/}\nolimits\!\left(3%
\mathop{\sin\/}\nolimits\phi\right)-\phi),
\theta_{{-}}(\phi)=\tfrac{1}{2}(\pi-\phi-\mathop{\mathrm{arcsin}\/}\nolimits\!%
\left(3\mathop{\sin\/}\nolimits\phi\right)).

These coalesce when

36.13.5|\phi|=\phi_{c}=\mathop{\mathrm{arcsin}\/}\nolimits\!\left(\tfrac{1}{3}\right)%
=19^{{\circ}}.47122.

This is the angle of the familiar V-shaped wake. The wake is a caustic of the “rays” defined by the dispersion relation (“Hamiltonian”) giving the frequency \omega as a function of wavevector \mathbf{k}:

36.13.6\omega(\mathbf{k})=\sqrt{gk}+\mathbf{V}\cdot\mathbf{k}.

Here k=|\mathbf{k}|, and \mathbf{V} is the ship velocity (so that \mathrm{V}=|\mathbf{V}|).

The disturbance z(\rho,\phi) can be approximated by the method of uniform asymptotic approximation for the case of two coalescing stationary points (36.12.11), using the fact that \theta_{{\pm}}(\phi) are real for |\phi|<\phi_{c} and complex for |\phi|>\phi_{c}. (See also §2.4(v).) Then with the definitions (36.12.12), and the real functions

36.13.7
u(\phi)=\sqrt{\dfrac{\Delta^{{1/2}}(\phi)}{2}}\left(\dfrac{1}{\sqrt{f_{{+}}^{{%
\prime\prime}}(\phi)}}+\dfrac{1}{\sqrt{-f_{{-}}^{{\prime\prime}}(\phi)}}\right),
v(\phi)=\sqrt{\dfrac{1}{2\Delta^{{1/2}}(\phi)}}\left(\dfrac{1}{\sqrt{f_{{+}}^{%
{\prime\prime}}(\phi)}}-\dfrac{1}{\sqrt{-f_{{-}}^{{\prime\prime}}(\phi)}}%
\right),

the disturbance is

See Figure 36.13.1.

See accompanying text
Figure 36.13.1: Kelvin’s ship wave pattern, computed from the uniform asymptotic approximation (36.13.8), as a function of x=\rho\mathop{\cos\/}\nolimits\phi, y=\rho\mathop{\sin\/}\nolimits\phi. Magnify

For further information see Lord Kelvin (1891, 1905) and Ursell (1960, 1994).