Parasitic ripple generation on short gravity waves (4 cm to 10 cm wavelengths) is
examined using fully nonlinear computations and laboratory experiments. Time-marching simulations show sensitivity of the ripple steepness to initial conditions,
in particular to the crest asymmetry. Significant crest fore–aft asymmetry and its
unsteadiness enhance ripple generation at moderate wave steepness, e.g. ka between
0.15 and 0.20, a mechanism not discussed in previous studies. The maximum ripple
steepness (in time) is found to increase monotonically with the underlying (low-frequency bandpass) wave steepness in our simulations. This is different from the sub-
or super-critical ripple generation predicted by Longuet-Higgins (1995). Unsteadiness
in the underlying gravity–capillary waves is shown to cause ripple modulation and
an interesting ‘crest-shifting’ phenomenon – the gravity–capillary wave crest and the
first ripple on the forward slope merge to form a new crest. Including boundary
layer efects in the free-surface conditions extends some of the simulations at large
wave amplitudes. However, the essential process of parasitic ripple generation is
nonlinear interaction in an inviscid flow. Mechanically generated gravity–capillary
waves demonstrate similar characteristic features of ripple generation and a strong
correlation between ripple steepness and crest asymmetry.