NUMERICAL SIMULATION OF WEAK TURBULENT KOLMOGOROV SPECTRUM
IN WATER SURFACE WAVES
Igor Lavrenov
Arctic and Antarctic Research Institute,
St.Petersburg, Russia, e-mail:<lavren@aari.nw.ru>
Don Resio,
Coastal and Hydraulics Labora tory, U.S. Army Engineer Research and Development Center, Halls Ferry
Road, Vicksburg, MS 39180,USA
Vladimir Zakharov (1,2,3)
(1) Landau Institute for Theoretical Physics, Moscow. 117334, Russia
(2) Department of Mathematics, University of Arisona, Tucson, AZ 857 21, USA
(3) Waves and Solitons LLC, 918 W.Windsong Dr., Phoenix, AZ 85045,USA
1. INTRODUCTION
Gravity waves in water surface are characterized by a small steepness value. It makes possible to apply the weak-
turbulence approach in order to find out the p roblem solution with the help of kinetic equation for energy spectrum.
This equation was formulated by K.Hasselmann (1962,1963) and V.Zakharov (1968). In terms of wave action
spectrum the equation is as follows:
N (k )
= Gnl = ∫∫∫ T (k,k 1 ,k 2 ,k 3 )δ(k +k 1 - k 2 -k 3 )δ (ω + ω - ω2 - ω3 )
1
t
{N 2 N 3 ( N + N 1 ) - N1 N ( N 2 + N 3 )}dk1 dk 2 dk 3
(1)
where N i = N ( ki ) is a spectral density of wave action; T ( k,k 1 , k 2 , k3 ) is a kernel function of non-linear wave
δ (ω) are the delta -functions describing a resonance interaction between four wave
interaction; δ (k ) and
components:
k +k1 = k 2 +k3 ;
(2a)
ω + ω1 = ω2 + ω3
(2b)
.
For gravity waves ω(k) =
gk , the value T ( k, k 1 , k2 , k 3 ) ~ k 3 is a homogenous function of the third order. An
T (k, k 1 , k2 , k3 ) can be found out in original papers (Hasselmann 1962, 1963; Webb 1978;
Zakharov 1999).
The equation (1) has been a subject of numerical modeling for almost three decades (Webb 1978, K.Hasselmann
1985; Resio and Perrie 1991; Polnikov 1993; Komen et al., 1994; Komatsu and Masuda 1996, Zakharov 1999,
Lavrenov 1998, 2001 etc.). However, some basic properties of this equation are not clarified till now.
Usually the equation (1) is considered to preserve standard constants of motion wave action, energy and
momentum: