If you want to see a tidal bulge propagating around the Earth in sync with the moon, take a look at
this animated gif that shows the movement of high and low tide around the amphidromes. There's a complicated rotary slosh within the ocean basins, driven by tidal forcing and Coriolis, but if you look at the Southern Ocean you can actually watch the southern amphidromes "hand off" the high tide to each other in a wave that moves continuously around the Earth from E to W.
And if you look at the tide magnitudes in
this gif, you can see that the rotary movement in the ocean is less evident than you might expect from the amphidrome view, because not all high tides are of the same magnitude - there's a strong E to W progression in the north Atlantic and north Pacific, as well as the one previously noted in the Southern Ocean, and considerable sloshing and swirling elsewhere.
This is the interface between the
equilibrium theory of tides (which deals with the idealized tidal bulges of Newton and Laplace), and the
dynamic theory of tides, which deals with how the real oceans on a rotating world respond to forcing from the tidal potential.
Grant Hutchison