Direct and Inverse Cascades in the Wind-Driven Sea

We offer a new form for the Snl term in the Hasselmann kinetic equation for squared wave amplitudes of wind-driven gravity wave. This form of Snl makes possible to rewrite in differential form the conservation laws for energy, momentum, and wave action, and introduce their fluxes by a natural way. We show that the stationary kinetic equation has a family of exact Kolmogorov-type solutions governed by the fluxes of motion constants: wave action, energy, and momentum. The simple ”local” model for Snl term that is equivalent to the ”diffusion approximation” is studied in details. In this case, Kolmogorov spectra are found in the explicit form. We show that a general solution of the stationary kinetic equation behind the spectral peak is described by the Kolmogorov-type solution with frequency-dependent fluxes. The domains of ”inverse cascade” and ”direct cascade” can be separated by a natural way. The spectrum in the universal domain is close to ω−4.