A physical model of the short wind wave spectrum in the wavelength range fr
om a few millimeters to few meters is proposed. The spectrum shape results
from the solution of the energy spectral density balance equation. Special
attention is paid to the description of the capillary range of the short wa
ve spectrum. It is assumed that in this range the spectrum shape is determi
ned mainly by the mechanism of generation of parasitic capillaries. This is
described as the cascade energy transfer from the gravity to the capillary
waves. Thus the capillary wave spectrum results through the balance betwee
n generation of capillaries and their viscous dissipation. The short gravit
y wave spectrum results through the balance between wind input and dissipat
ion due to wave breaking. A parameterization of wind input is obtained in p
art 1 of the present paper. To describe the dissipation due to wave breakin
g, the approach developed by Phillips [1985] is used. The spectral rate of
energy dissipation is presented in the form of a power dependence of the ra
tio of the saturation spectrum to some threshold level. It is further shown
that the threshold level depends on the drift current shift in the water v
iscous sublayer, which affects the energy losses by wave breaking. To obtai
n a short wave spectrum which is valid in the whole wavenumber domain, the
capillary and the short gravity wave spectra are patched in the vicinity of
the wavenumber corresponding to the minimum phase velocity. This short wav
e spectrum is incorporated into the wind over waves coupled model developed
in part 1 of the present paper. The measured statistical properties of the
sea surface related to the short waves, such as the spectral shape of omni
directional and up-wind spectra, their wind speed dependence and angular sp
reading, and the wind speed dependence of integral mean square slope and sk
ewness parameters, are well reproduced by the model. Also the model well re
produces the measured wind speed dependence of the drag coefficient and of
the coupling parameter.