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a reduced model for internal waves interacting with submarine ...

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Also, recall that<br />

K1=E(η n , u n 1 ),<br />

KK1=F(η n , u n 1 ),<br />

u 1k1 =Ψ(η n + 0.5∆tK1, V n + 0.5∆tKK1),<br />

K2=E(η n + 0.5∆tK1, u 1k1 ),<br />

KK2=F(η n + 0.5∆tK1, u 1k1 ),<br />

u 1k2 =Ψ(η n + 0.5∆tK2, V n + 0.5∆tKK2),<br />

K3=E(η n + 0.5∆tK2, u 1k2 ),<br />

KK3=F(η n + 0.5∆tK2, u 1k2 ),<br />

u 1k3 =Ψ(η n +∆tK3, V n +∆tKK3),<br />

K4=E(η n +∆tK3, u 1k3 ),<br />

KK4=F(η n +∆tK3, u 1k3 ).<br />

Notice that the projection from (η, V) back to u 1 must be done after each stage.<br />

These intermediate values are denoted by u 1ki , i=1, 2, 3.<br />

Now we will specify how to deal <strong>with</strong> the operatorΨin order to recover u 1 in<br />

terms of V andη. Since the Fast Fourier Trans<strong>for</strong>m (FFT) of a Hilbert trans<strong>for</strong>m<br />

is easily computed, as well as the FFT <strong>for</strong> aξ-derivative, we can go to frequency<br />

space and solve u 1 in terms of V <strong>for</strong> the linear and constant coefficients relation<br />

that appears in Table 4.2 <strong>for</strong> both LFM and WNFM. In Fourier space we have<br />

̂V(k)=<br />

(<br />

1+ √ β ρ ( ))<br />

2 kπ<br />

ρ 1 l coth kπh2<br />

û 1 (k)<br />

lL<br />

62

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