The velocity, c, of a simple sinusoidal surface water wave is described by, where L is the wavelength and d the water depth:
[tex]c = \sqrt {\frac{{gL\tanh \left( {\frac{{2\pi d}}{L}} \right)}}{{2\pi }}}[/tex]
Note that when d > L /2
[tex]\tanh \left( {\frac{{2\pi d}}{L}} \right) \approx 1[/tex]
so the velocity for deep water reduces to
[tex]c = \sqrt {\frac{{gL}}{{2\pi }}}[/tex]
and when d << L/2
[tex]\tanh \left( {\frac{{2\pi d}}{L}} \right) \approx \left( {\frac{{2\pi d}}{L}} \right)[/tex]
So the velocity becomes
[tex]c = \sqrt {gd}[/tex]
This is because the water particles are moving in (nearly) circular orbits in deep water. As the water shoals the bottom exerts a drag which elongates the orbit to an ellipse, which gets flatter and flatter with shoaling.