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along the interface in the positive x direction would have the same form as a surface
wave, i.e.:
z
¼
A 0 sin
ð
kx
ot
Þ:
ð
4
:
16
Þ
The corresponding velocity potential describing motion within the two layers may be
obtained by essentially the same methods as used for the surface waves (see Phillips,
1966 , p. 167) to give:
oA 0
k
cosh kz
sinh kh 1 cos
upper layer
:
f
¼
ð
kx
ot
Þ
0
>
z
>
h 1
ð
4
:
17
Þ
ð
þ
Þ
oA 0
k
cosh k
h
z
lower layer
:
f
¼
cos
ð
kx
ot
Þ
h 1 >
z
>
h 2
sinh kh 2
from which we can find expressions for the horizontal and vertical particle velocities
as in the surface wave case. The phase speed c of the waves is given by:
o 2
k 2 ¼
g 0
k ð
coth kh 2 Þ 1
c 2
¼
coth kh 1 þ
ð
4
:
18
Þ
where g 0 ¼
is the reduced gravity.
In many situations in shelf seas, we are concerned with waves of long period
(up to the semi-diurnal (
g
ð= 0 Þ
24 hours) periods). For such
waves, the wavelength is long compared with the depth (
12 hours) and diurnal (
l ≫
h) so that kh
1and
kh 2 Þ 1 etc. so Equation (4.18) then simplifies to:
we can approximate coth kh 2 ð
h 1 h 2
h 1 þ
h 1 h 2
h
c 2
g 0
g 0
¼
h 2 ¼
ð
4
:
19
Þ
where h
¼
h 1 þ
h 2 is the water column depth. If, in addition, the upper layer thickness
g 0 h p . This is of the
same form as the expression for the speed of long surface waves, but the speeds
involved are much lower, mainly because g 0 /g
h 1
h, the phase speed can be further approximated by c
¼
10 3 which makes the
¼ D
r/r 0
internal waves travel
30 times slower than their surface counterparts.
4.2.2
Particle motions in internal waves
The motion described by the velocity potential of Equation (4.17) , termed the lowest
mode or the first vertical mode, is an important reference solution which we will now
explore in more detail. The particle velocities u and v are readily obtained by
differentiation of the velocity potentials in the two layers. For example, in the bottom
layer (
h 2 <
z
<
h 1 ) at a particular location (x
¼
0) we have:
¼ @
f
oA 0 cosh k
ð
h
þ
z
Þ
x ¼
u
sin ot
@
sinh kh 2
ð
4
:
20
Þ
¼ @
f
@
oA 0 sinh k
ð
h
þ
z
Þ
w
z ¼
cos ot
sinh kh 2
 
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