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Transcript
Journal of Oceanography
Vol. 52, pp. 353 to 357. 1996
Shallow Water Gravity Waves: A Note on the Particle Orbits
KERN E. KENYON
4632 North Lane, Del Mar, CA 92014-4134, U.S.A.
(Received 4 July 1995; in revised form 2 November 1995; accepted 8 November 1995)
When surface gravity waves of small amplitude progress in shallow water of
constant mean depth, the fluid particle orbits are observed to be oval, where the
longer axis of the oval is parallel to the flat bottom, and at the bottom the orbits are
straight lines. Potential flow, upon which the standard wave theory is based,
predicts that the oval orbits are ellipses, but by a rather lengthy mathematical
procedure that is founded on the questionable assumption of irrotationality. Using
a more elementary and physical method, that does not employ the irrotational
assumption, the elliptical orbits can be understood much more easily. The elementary method features a balance of two oppositely directed forces on each fluid
particle: the outward centrifugal force and the inward pressure force.
1. Introduction
When gravity waves of infinitesimal amplitude progress over the surface of deep water, the
fluid particles are observed to move in circles in the frame of reference fixed to the bottom. Deep
water means that the wave length is smaller than the average total water depth. Actually fluid
particles are not observed, but the idea of circular orbits, which has been around for a long time,
is confirmed by streak photographs (Sommerfeld, 1964) or movie films (Bryson) of small
neutrally buoyant particles in laboratory wave tanks.
In shallow water, for which the water depth is less than one wave length, observations show
that the particles no longer move in circles but in ovals, where the longer axis of the oval is parallel
to the bottom or to the mean surface. At the flat bottom the orbits are straight lines. The notion
that these oval paths might be ellipses probably comes more from theory than from observations.
I am not aware of any measurements that show that the particle orbits of shallow water waves are
indeed ellipses.
The standard (potential flow) theory of shallow water waves produces elliptical orbits, but
considerable analytic effort is required to get to this point. First the Eulerian potential flow
problem must be set up by a perturbation analysis on the nonlinear equations of motion and the
nonlinear boundary conditions. Then after the linearized potential problem is solved, the particle
orbits must be obtained by equating the Lagrangian and Eulerian velocities through a Taylor
expansion.
Also the whole method is founded on the questionable assumption of irrotationality.
Irrotationality means that the curl of the velocity must be zero everywhere and always. The
irrotational assumption, though sometimes convenient, has been found to be unnecessary for the
derivation of several characteristics of surface gravity waves in deep water (Kenyon, 1991), such
as the dispersion relation and the exponential decrease with depth of the wave motion and
pressure variation. It will be shown below that the elliptical particle orbits of shallow water waves
can be derived also without employing the irrotational assumption.
This investigation uses elementary procedures, featuring a balance of forces, in order to
354
K. E. Kenyon
arrive at the orbits of fluid particles in shallow water waves. One force, in the balance of two
oppositely directed forces, is the outward centrifugal force acting on the fluid particles as they
move around their curved orbits. The inward force is a pressure force that is related to the
differences in height of the surface and to the vertical acceleration of the fluid. Results obtained
here are in complete agreement with those of the standard theory, but the present labor-saving
method facilitates a greater and more immediate understanding of the phenomenon.
Another distinct advantage of the force balance method over the potential flow formulation
comes from the spatially local character of the force balance on the orbiting fluid particles. In
order to solve the potential problem (i.e. Laplace’s equation) it is necessary to assume that the
sinusoidal wave train is horizontally infinite in extent, but no such assumption need be made in
balancing the two forces on a particle. Therefore the force balance method is much more readily
adaptable to wave trains of finite extent or even to solitary waves.
The present method might be called into question because of its bold use of the centrifugal
force. Currently in physics the centrifugal force enjoys an ambiguous status. Sometimes it is
brought out into the open, for example in problems where circular motion occurs, but often it is
considered to be a fictitious force which is best avoided. However, recently (Kenyon, 1994) a
force balance for the motion of a planet around the sun, involving the outward centrifugal force
and the inward gravitational force component normal to the orbital path, has produced theoretically
all three of Kepler’s empirical laws, the elliptical orbits being one (the first law), and these results
therefore support the reality of the centrifugal force. Consequently there is no hesitation about
using the centrifugal force here.
2. Force Balance of Surface Particles
A surface gravity wave progresses in shallow water of constant mean depth h. Assume that
the wave has a sinusoidal form ζ = asin(kx – ωt), where a is the infinitesimal amplitude, k the wave
number, ω the angular frequency, and ζ is the elevation of the surface above the mean level (z
= 0). [The assumption of a sinusoidal wave form is not necessary here, but it is convenient. The
property of a sinusoid that it extends to infinity in two directions is not used at all.] Shallow water
means kh ≤ 1. Infinitesimal amplitude means the amplitude is much less than the water depth.
Consider a fluid particle at the surface and at the position where the surface has maximum
slope. At this location the velocity of the surface particle has only a vertical component, and for
the moment it does not matter whether the vertical velocity is up or down. It is evident, because
the particle velocity must equal the velocity of the surface, that the magnitude of the vertical
velocity w will be |w| = |dζ/dt| = ωa. There will be a centrifugal force, of magnitude ρ(ωa)2/R,
acting on this vertical velocity which will point in the horizontal direction, where R is the radius
of curvature of the orbit. The counterbalancing pressure force in the horizontal direction has
magnitude ρgka (Kenyon, 1991). Carrying out the balance of the centrifugal and pressure forces,
and canceling the constant density ρ from both sides, gives
(ω a )2
R
= gka.
(1)
For shallow water waves of infinitesimal amplitude the phase speed c = ω/k = (gh)1/2. This
well-known relationship can be understood independent of the irrotational assumption also
(Kenyon and Sheres, 1990); in fact it can be derived from a balance of two pressure forces (static
Shallow Water Gravity Waves: A Note on the Particle Orbits
355
and dynamic), in the reference frame that makes the wave form steady, by following a method
due to Einstein (1916). After incorporating the equation for the phase speed (1) becomes
R = ( kh )a.
(2 )
Since kh ≤ 1, then (2) gives R ≤ a. Thus the radius of curvature, at the position of greatest slope,
is less than the wave amplitude, whereas for deep water waves with circular particle orbits the
radius of curvature is constant and equal to the amplitude.
Consider next a fluid particle at the surface of a wave crest. The downward acceleration for
a sinusoidal wave, d2ζ/dt2 , has magnitude ω2a. By Newton’s second law there is a downward
force which causes this downward acceleration, and it must be a pressure force (Kenyon, 1991).
The upward force is the centrifugal force. Therefore the balance of forces for the surface particle
at the crest is
ω 2a =
u2
R
(3)
where the density has been cancelled from both sides. The objective now is to calculate the radius
of curvature at the crest. First the horizontal component of the particle velocity, u, must be
evaluated.
The particle speed at the crest is conveniently computed by starting in the frame of reference
that moves with the phase velocity of the wave (Kenyon and Sheres, 1990). A commonly used
assumption for shallow water waves of infinitesimal amplitude is that the horizontal velocity is
independent of depth below the surface. Then by conservation of mass between a cross-section
where the surface elevation is zero and a cross-section at a crest, ch = u′(h + a), where u′ is the
horizontal fluid speed beneath the crest in the reference frame moving with the wave. Now
converting back to the fixed frame the particle speed below the crest is u = c – u′, or
a
1/ 2 a
u ≈ c  = ( gh )   .
 h
 h
( 4)
Putting (4) and the relationship c = ω/k = (gh)1/2 , already used above, into (3) gives the end
result
2
1
R = a  .
 kh 
(5)
Since kh ≤ 1 for shallow water, then (5) shows R ≥ a. Therefore at the crest the radius of curvature
is greater than the wave amplitude. In fact as the ratio of the wave length to the water depth
steadily increases, the radius of curvature at the crest increases faster than the radius of curvature
decreases at the position of maximum slope, as can be seen from (2) and (5).
3. Comparison with Potential Theory
It is easy enough to demonstrate that the radius of curvature at the crest in (5) and that at the
356
K. E. Kenyon
position of maximum slope in (2) agree exactly with those which can be computed from the
elliptical orbits produced by the standard potential theory. For this purpose the convenient
formula for the radius of curvature is (Thomas, 1953)
2
 dx 2
dz 
R =   +   
 dt   dt  
3/ 2
 dx d 2 z dz d 2 x 
−


 dt dt 2 dt dt 2 
(6)
and the parametric equations for the orbits of surface particles in shallow water waves are
(Defant, 1961)
a 
sin ωt,
x=
 tanh kh 
z = a cos ωt.
( 7)
To arrive at Eqs. (2) and (5), insert (7) into (6), take kh small compared to 1, and select the phase
for the crest (ωt = 0) and for the position of maximum slope (ωt = π/2).
4. Surface Particle Orbits
So far the elementary and classical theories agree at the extreme horizontal and vertical
positions of the particle orbits. The question now is, can it be shown by elementary means that
the orbits are actually ellipses?
A harmonic motion of frequency ω and amplitude a has been assumed from the start, and
the maximum vertical and horizontal velocities of the surface particles have been deduced or
calculated above to be wmax = ωa and umax = ωa/kh, respectively. Therefore the particle orbits are
given by a time integration of the equations
dz
= ωa sin ωt,
dt
( 8)
dx ωa
=
cos ωt.
dt kh
The integration of Eq. (8) can be put into the form for the ellipse
2
2
 x  + z  =1
 A  B
( 9)
where A = a/kh and B = a.
5. Subsurface Orbits
The particle orbits beneath the surface are ellipses too, but they degenerate to straight lines
at the level bottom (z = –h). This can be seen by first considering the force balance on particles
below the crest. Since the vertical acceleration of the fluid particles must go to zero at the bottom,
Shallow Water Gravity Waves: A Note on the Particle Orbits
357
while the horizontal velocity remains constant, then the radius of curvature of the orbits must
become infinitely large at the bottom as can be seen from Eq. (3). More explicitly, if the vertical
acceleration decreases linearly with increasing depth, which is a good approximation in shallow
water, then (3) becomes
u2
z
ω 2 a 1 +  =
 h R
(10 )
and by incorporating (4) as before, Eq. (5) changes to
1
R = a 
 kh 
2
1
1+
z
h
(11)
showing that R → ∞ as z → –h.
Next it can be shown from the force balance that the radius of curvature of the particles below
the maximum wave slope goes to zero at the bottom. This can be seen from Eq. (1) with the
addition of the constraint that the vertical velocity must vanish at the bottom while the horizontal
pressure gradient remains finite there. Therefore when the radius of curvature at the bottom
becomes infinite below the crest and trough and zero below the maximum slope, the elliptical
orbits have degenerated into straight lines.
References
Bryson, A. E.: Waves in Fluids. National Committee for Fluid Mechanics Films, Encyclopaedia Britannica Educational Corporation, 425 North Michigan Avenue, Chicago, IL 60611.
Defant, A. (1961): Physical Oceanography. Pergamon Press, NY, Vol. 2, p. 18, 598 pp.
Einstein, A. (1916): Elementare theorie der wasserwellen und des fluges. Naturwissenschaften, 24, 509–510.
Kenyon, K. E. (1991): The cyclostrophic balance in surface gravity waves. J. Oceanogr. Soc. Japan, 47, 45–48.
Kenyon, K. E. (1994): Kepler’s laws deduced from a force balance. Phys. Essays, 7, 464–467.
Kenyon, K. E. and D. Sheres (1990): Stable gravity wave of arbitrary amplitude in finite depth. Int. J. Theor. Phys.,
29, 101–108.
Sommerfeld, A. (1964): Mechanics of Deformable Bodies. Academic Press, NY, p. 181, 396 pp.
Thomas, G. B. (1953): Calculus and Analytic Geometry. Addison-Wesley Publishing Co., Inc., Cambridge, MA, p.
405, 822 pp.