Numerical methods are employed to study the equations of directional approx
imation, which were derived previously by Zakharov and Smilga [10] for Hass
elmann's kinetic equation and which were transformed by Zaslavskii [12] to
the form that admits self-similar solutions. Numerical solutions to Zaslavs
kii's equations are obtained in a limited hand of wave numbers. It is shown
that, in the region of-a spectral peak, the numerical solutions are in clo
se agreement with the analytic solutions derived by Zaslavskii [12]. Howeve
r, these solutions differ in the region away;from the spectral peak. A comp
arison of the above solutions with the numerical solution of the initial ki
netic equation obtained previously by the author [9] testifies to their goo
d agreement and to-a wide range of validity of the directional approximatio
n. The results of this comparison of solutions make it possible to give an
efficient analytic approximation for a self-similar spectrum of swell, whic
h is suitable for use: in numerical models of wind waves.