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Initial Conditions

The amplitudes of initial waves were given by the Wallops type spectrum in wavenumber space transformed through the linear dispersion relation.

\begin{displaymath}
S(k)\, dk=\frac{\alpha}{2} H_{1/3}^2\kappa^{-{m\over2}}
\ex...
...th} k_ph}}
\left[1+\frac{2kh}{{\rm sh} 2kh}
\right]
\, dk
\end{displaymath} (4)


\begin{displaymath}
\kappa={k {\rm th} kh}/{k_p {\rm th} k_ph}
\end{displaymath} (5)

where, $m$ the spectral bandwidth parameter, $k_p$ the peak wavenumber of spectra, $h$ the water depth and $\alpha$ is a constant satisfying a following relation with $H_{1/3}$:
\begin{displaymath}
H_{1/3}=4.004\sqrt{\int_0^\infty S(k)dk}.
\end{displaymath} (6)

Eq.(4) with $m$=5 and $k_ph$=$\infty$ is equivalent to JONSWAP spectra and the shape of spectrum is getting narrower as increasing the value of $m$. The Wallops spectrum is evaluated as a function of spectrum bandwidth $m$ only. The phase constants of the initial waves were assumed a random phase approximation. This assumption is very important for simulating realistic random waves. A further important point is that if the phase is given factitiously(e.g. frequency wave focusing), it is possible to generate a freak wave like surface profile at an arbitrary time and location. However, such approach is out side of the scope of this study.

The computations were made in the periodic space having the length of $256L_p$. Initial wave statistics were comprised with fixed characteristic wave steepness: $k_pa$=0.14 and spectrum band width:$m$=10, 20, 30, 40, 60, 80 and 100 as shown in Figure 1. Here, $a$ is a half of $H_{1/3}$, and $L_p$ and $T_p$ are the wave length and wave period of spectral peak mode, respectively. The water depth was chosen as $k_ph$=$\infty$(deep-water), 3.0, 2.0, 1.36, 1.0. The total time integration was calculated up to $t$=$100T_p$.

Figure 2: Temporal evolutions of the Fourier spectra of the simulated wave train which has steepness $k_pa$=0.14 and spectrum bandwidth $m$=10, initially.
\begin{figure*}\wIncGraphSubcap{figures/random_spect_timeseries_m30deep.eps}{12....
...spect_timeseries_m30deep_2nd.eps}{12.0}
{Second-order solution}
\end{figure*}


next up previous
Next: Numerical Results and Discussions Up: Numerical Method Previous: Governing Equations

2005-11-21