MOHIBB MALIK

one wave, six theories

Ocean Waves

A single wave propagating over a still-water line, with arrows showing each water particle's instantaneous velocity at several depths — watch the orbital motion fade out toward the seabed. Pick a theory to drive that wave: Linear (Airy), Stokes 2nd- or 5th-order, cnoidal, solitary, or trochoidal (Gerstner). Below that, the same height/period/depth re-evaluated under all six at once, overlaid — and below that, a real irregular sea built from a JONSWAP spectrum of randomly-phased components.

01 Wave

1.0
8.0

Height and period drive both the single-wave view above and the theory comparison below.

02 Water depth

40
Regime
Phase speed c
Wavelength λ
Breaking limit

Breaking limit is the Miche (1944) criterion Hb = 0.142·λ·tanh(kh) — the steepest a wave of this wavelength and depth can get before it breaks. Shown as the current height's share of that limit.

03 Theory & arrows

04 Theory comparison

All six theories use the same height, period, and depth from the panels above — only the shape (and, above, the velocity field) each one predicts differs.

05 Playback

1.0

06 Irregular sea

1.5
8.0
3.3

γ=1 is the Pierson-Moskowitz spectrum (a fully developed sea); γ≈3.3 is the more peaked JONSWAP default for a developing sea. Uses its own depth from panel 02.

A single wave above a still-water line, with arrows showing how far each theory thinks particle motion reaches below the surface; the same wave's height, period, and depth re-evaluated under all six theories at once below that; and below that, an irregular sea built from many randomly-phased components drawn from a JONSWAP spectrum. For the equations behind every term, open .