Parasitic ripple generation on short gravity waves (4 cm to 10 cm wavelengt
hs) is examined using fully nonlinear computations and laboratory experimen
ts. Time-marching simulations show sensitivity of the ripple steepness to i
nitial conditions, in particular to the crest asymmetry. Significant crest
fore-aft asymmetry and its unsteadiness enhance ripple generation at modera
te wave steepness, e.g. ka between 0.15 and 0.20, a mechanism not discussed
in previous studies. The maximum ripple steepness (in timew) is found to i
ncrease monotonically with the underlying (low-frequency bandpass) wave ste
epness in our simulations. This is different from the sub- or super-critica
l ripple generation predicted by Longuet-Higgins (1995). Unsteadiness in th
e underlying gravity-capillary waves is shown to cause ripple modulation an
d an interesting 'crest-shifting' phenomenon - the gravity-capillary wave c
rest and the first ripple on the forward slope merge to form a new crest. I
ncluding boundary layer effects in the free-surface conditions extends some
of the simulations at large wave amplitudes. However, the essential proces
s of parasitic ripple generation is nonlinear interaction in an inviscid fl
ow. Mechanically generated gravity-capillary waves demonstrate similar char
acteristic features of ripple generation and a strong correlation between r
ipple steepness and crest asymmetry.