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With this choice, φ now satisfies the Laplace equation in the interior of the
fluid and the bottom boundary condition. Let's write out what we have
for this Fourier mode so far:
φ ( x, y, z, t )= φ ij ( t ) e 12 π ( ix + jz ) /L e ky + e 2 kH e −ky . (13.1)
All that's left to determine is the time dependence of the potential φ ij ( t )
and the height field h ij ( t ), and the only equations we have left are the
boundary conditions at y =0: ∂φ/∂t =
gh and ∂h/∂t = ∂φ/∂y .These
two boundary equations at the free surface become (after cancelling out
the common e 12 π ( ix + jz ) /L factor):
∂ φ ij
∂t
gh ij ,
(1 + e 2 kH )=
(13.2)
∂h ij
∂t
φ ij ( k
ke 2 kH ) .
=
Now, differentiate the second equation with respect to time, and replace
the ∂ φ ij /∂t term with the first equation, to get
2 h ij
∂t 2
e 2 kH
kg 1
1+ e 2 kH h ij .
=
(13.3)
This is another simple ordinary differential equation, with general solution
consisting of yet more Fourier sinusoids, e 1 ω k t and e 1 ω k t where the
wave frequency ω k (how fast the wave is going up and down, no relation
at all to vorticity) is given by
kg 1
e 2 kH
1+ e 2 kH .
ω k =
(13.4)
Before going on to the full solution, and accompanying numerical method,
it's instructive to pause a moment and reinterpret this height field solution.
Writing out the one of the components of the height field gives
h ( x, z, t )= e 1 ω k t e 12 π ( ix + jz ) /L
= e 1( ( x,z ) −ω k t )
= e 1 [( x,z ) −c k tk ] ,
(13.5)
where k = k/k is the unit-length direction of the wave (normal to the crests
and troughs) and c k
is the wave speed, defined as
ω k
k
c k =
g (1
(13.6)
e 2 kH )
k (1 + e 2 kH ) .
=
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