A small-amplitude deep-water wave with surface elevation has dispersion relation and a velocity potential that decays as below the surface.
A deep-water gravity wave has dispersion . An observer moving with nonzero speed samples Fourier phases . The stationary phase method selects the points where their derivatives vanish, which gives the displayed wavenumbers. Their group velocity matches the observer's velocity. For real even initial displacement with a nonzero Fourier coefficient there, the resulting signal has leading size and phase . If the initial coefficient vanishes, that leading term is absent; a stationary observer does not select a finite nonzero wavenumber by this rule.
For two wave periods emitted together at one location, deep-water group velocity is . A distant observer sees the shorter period later, with . This yields the displayed range estimate. Different emission times, a moving storm, finite-depth dispersion, currents and refraction are possible confounders; the propagation calculation alone does not establish a unique source range without these assumptions.
For elevation , depth-integrated kinetic energy per surface area is . Wavelength-averaged excess gravitational energy is . Conservation gives in the inviscid gravity-only model.
For an impulsive distant source of deep-water gravity waves, a component of period travels at group velocity . Its arrival at distance obeys the displayed law, so inverse period increases linearly with arrival time. Two arrivals determine both and . Finite source duration, currents, refraction and passage through sea ice can invalidate the simple inversion.
For small kinematic viscosity , the mean viscous dissipation per unit horizontal area is . Since the mean wave energy is , the amplitude obeys
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