Wave Theory: Circular Orbits to Irrotational Motion & Mass Transport, Exams of Local Government Studies

The development of wave theory, from the circular orbits of water particles in infinite depth to the irrotational motion and mass transport in waves of finite height. the works of Laplace, Airy, Stokes, and their significant contributions to understanding wave velocity, orbital motion, and the relationship between wave period, wave length, and water depth.

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CHAPTER
2
ELEMENTS OF WAVE THEORY
R. L. WIegel and
J.
W Johnson
Respectively, Institute of
Engineermg
Research,
and DiviSlOn
of MechanIcal
Engmeering
UmversIty
of
Callforma
Berkeley,
Callforma
INTRODUCTION
The
first
known
mathematical
solution
for
finite
height,
periodic
waves
of
stable
form
was
developed
by
Gerstner
(1802).
From
equations
that
were
developed,
Gerstner
(1802)
arrived
at
the
conclusion
that
the
surface
curve
was
trochoidal
in
form.
Froude
(1862)
and
Rankine
(1863)
developed
the
theory
but
in
the
opposite
manner,
i.e.,
they
started
with
the
assumption
of
a
trochoidal
form
and
then
de-
veloped
their
equations
from
this
curve.
The
theory
was
developed
for
waves
in
water
of
infinite
depth
with
the
orbits
of
the
water
particles
being
circular,
de-
creasing
in
geometrical
progression
as
the
distance
below
the
water
surface
in-
creased
in
arithmetical
progression.
Recent
experiments
(Wiegel,
1950)
have
shown
that
the
surface
profile,
represented
by
the
trochoidal
equations
(as
well
as
the
first
few
terms
of
Stokes'
theory),
closely
approximates
the
actual
profiles
for
waves
traveling
over
a
horizontal
bottom.
However
the
theory
necessitates
molecu-
lar
rotation
of
the
particles,
while
the
manner
in
which
waves
are
formed
by
con-
servative
forces
necessitates
irrotational
motion.
The
first
satisfactory
treatment
of
two
dimensional
wave
motion
in
water
of
arbitrary
depth
was
given
by
La
Place
(1776)
for
waves
of
small
amplitude.
Airy
(1845)
developed
an
irrotational
theory
for
waves
traveling
over
a
horizontal
bottom
In
any
depth
of
water.
This
theory
was
developed
for
waves
of
very
small
height.
Airy
(1845)
showed
that
the
velocity
of
propagation
of
the
wave form was
dependent
upon
the
wave
length
as
well
as
upon
the
water
depth.
stokes
(1847)
presented
an
approximate
solution
for
waves
of
finite
height
which
satisfied
the
boundary
conditions
of
waves
In
water
of
uniform
depth
and,
in
addition,
required
irrotational
motIon.
The
series
was
to
the
thIrd
approximation
for
finite
depths,
or
to
the
fifth
approximation
for
infinite
depths,
but
there
was
no
proof
of
their
convergence.
The
most
interesting
features
of
the
solution,
apart
from
the
irrotational
motion,
were,
first,
the
dependency
of
the
wave
ve-
locity
upon wave
height
as
well
as
upon wave
length
and
water
depth
and,
second,
the
fact
that
orbital
motion
of
the
particles
was
open
rather
than
closed,
indI-
cating
a mass
transport
in
the
direction
of
wave
travel.
Experiments
(Mitchim,
1940)
have
shown
both
of
these
findings
to
be
correct.
Levi-Civita
(1925)
proved
that
Stokes'
series
was
convergent
for
"deep-water"
waves
and
Struik
(1926)
proved
that
it
was
convergent
for
"shallow-water"
waves.
Reynolds
(1877)
and
Rayleigh
(1877)
worked
on
the
problem
of
the
difference
between
the
energy
transmission
velocity
of
a wave
group
and
the
velocity
of
the
wave
form.
They
concluded
that
the
energy
of
the
group
of
waves was
propagated
with
a
velocity
less
than
that
of
the
individual
waves.
In
deep
water,
the
"group"
velocity
was
found
to
be
one-half
the
wave
velocity.
The
problem
of
the
maximum
steepness
(the
ratio
of
the
wave
height
to
its
length)
that
a wave
could
attain
without
breaking
was worked
on
by
Stokes
(1847),
Michell
(1893),
and
Havelock
(1918).
Their
conclusions
were
in
close
agreement.
A
crest
angle
of
120
degrees,
or
a
steepness
of
H/L =
0.142,*
was
found
to
be
the
theoretical
limit.
Recently,
many
field
and
laboratory
studies,
as
well
as
analytical
studies,
have
been
made.
These
observations,
together
with
the
mathematical
studIes,
lead
*See
list
of
symbols.
5
pf3
pf4
pf5
pf8
pf9
pfa
pfd
pfe
pff

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CHAPTER 2

ELEMENTS OF WAVE THEORY

R. L. WIegel and J. W Johnson Respectively, Institute of Engineermg Research, and DiviSlOn of MechanIcal Engmeering UmversIty of Callforma Berkeley, Callforma

INTRODUCTION

The first known mathematical solution for finite height, periodic waves of stable form was developed by Gerstner (1802). From equations that were developed, Gerstner (1802) arrived at the conclusion that the surface curve was trochoidal in form. Froude (1862) and Rankine (1863) developed the theory but in the opposite manner, i.e., they started with the assumption of a trochoidal form and then de- veloped their equations from this curve. The theory was developed for waves in water of infinite depth with the orbits of the water particles being circular, de- creasing in geometrical progression as the distance below the water surface in- creased in arithmetical progression. Recent experiments (Wiegel, 1950) have shown that the surface profile, represented by the trochoidal equations (as well as the first few terms of Stokes' theory), closely approximates the actual profiles for waves traveling over a horizontal bottom. However the theory necessitates molecu- lar rotation of the particles, while the manner in which waves are formed by con- servative forces necessitates irrotational motion.

The first satisfactory treatment of two dimensional wave motion in water of arbitrary depth was given by La Place (1776) for waves of small amplitude. Airy (1845) developed an irrotational theory for waves traveling over a horizontal bottom In any depth of water. This theory was developed for waves of very small height. Airy (1845) showed that the velocity of propagation of the wave form was dependent upon the wave length as well as upon the water depth.

stokes (1847) presented an approximate solution for waves of finite height which satisfied the boundary conditions of waves In water of uniform depth and, in addition, required irrotational motIon. The series was to the thIrd approximation for finite depths, or to the fifth approximation for infinite depths, but there was no proof of their convergence. The most interesting features of the solution, apart from the irrotational motion, were, first, the dependency of the wave ve- locity upon wave height as well as upon wave length and water depth and, second, the fact that orbital motion of the particles was open rather than closed, indI- cating a mass transport in the direction of wave travel. Experiments (Mitchim,

  1. have shown both of these findings to be correct.

Levi-Civita (1925) proved that Stokes' series was convergent for "deep-water" waves and Struik (1926) proved that it was convergent for "shallow-water" waves.

Reynolds (1877) and Rayleigh (1877) worked on the problem of the difference between the energy transmission velocity of a wave group and the velocity of the wave form. They concluded that the energy of the group of waves was propagated with a velocity less than that of the individual waves. In deep water, the "group" velocity was found to be one-half the wave velocity.

The problem of the maximum steepness (the ratio of the wave height to its length) that a wave could attain without breaking was worked on by Stokes (1847), Michell (1893), and Havelock (1918). Their conclusions were in close agreement. A crest angle of 120 degrees, or a steepness of H/L = 0.142,* was found to be the theoretical limit.

Recently, many field and laboratory studies, as well as analytical studies, have been made. These observations, together with the mathematical studIes, lead *See list of symbols.

COASTAL ENGINEERING

to the conclusion that Stokes' irrotational theory represents the natural phenomena more closely than the other theories.

Waves in nature vary considerably in height and period over a relatively short length of time at any pOint of observation. In a generating area, the wave charac- teristics show the maximum variability; however, even after the waves have passed into a region of relative calm, considerable variations in wave characteristics exist. In theoretical problems, such variability cannot be treated mathematlcally and certain idealized conditions must be assumed. Accordingly, the flrst step in the analysls of oscillatory waves is to study the behavior of single wave trains of unlform period and amplitude as they progress in water of constant depth. Present-day wave theory deals 'nth periodic waves of stable form in which all ele- ments of the wave profile advance with the same velocity relative to the undis- turbed water. Complete development of the various analyses of Lamb (1932), Stokes (1847), Gerstner (1802), and others are not presented herein as they are readily available in the original references.

WAVES OF SMALL AMPLITUDE

If waves are of small amplitude compared to their length and to the depth of the water, the wave profile closely approximates a sine curve. The equation for motion (Lamb, 1932), considering both gravity and surface tension, is:

(gL/2 rr + 2 7ro/pL) tanh 27r"d/L (1)

For water deeper than one-half the wave length, tanh 2 rr^ d/L is almost equal to 1 and the equatlon reduces to:

0 z (^00) '"If) a: '"II. ~ '"'"...

I- <> 0 ...J '"> '"> ~ 0: '"~ ~ II. '"'" 0

24

20

16

12

08

04

o

o

1'-" l 'II I' , f f

~PE CEN^ DIFFERENPE / c!. 9 Lo^ .~^ ,/

2iT (Lo I~ /'

~ V

\ V

\

V/

l! ~ ~~ (^) 2rI9Lo^ I'--I---

" (^) k::~ =~

  • -. (^) -- -- --

(^02 04) 0.6 08 DEEP WATER WAVE LENGTH, FEET

20

I L, :jfl"

I

I

4 , -'

I

] r 2 " 1=

Io - 1=

~

'~+ ~~'"

  • , 8 ~ .:J ,o (^) - '" ..J 6 ~

2

o

'"<>z '"a: ...^ '"... is I- z '"<> a: '"II. 10

Fig. 1. Effect of surface tension on deep water wave velocity in fresh water at 70 oF.

The relatlve effects on ve- locity of the gravity and the sur- face tension components for deep- water waves are presented in Fig. 1. Experimental data by Chinn (1949) and Kaplan (1950) verifies the equation. It can be seen that for any wave over a foot in length, the effect of surface tension may be neglected. In practice, these small waves are usually called ripples as distinguished from the longer waves •

Neglecting the effect of sur- face tenSion, the equation for ve- loclty of propagation of gravity waves (Airy, 1845; Lamb, 1932)

C^2 = (gL/27r) tanh 21fd/L (^) (3)

and for "deep-water:"

Co 2

= gLo/21f (^ 4a)

or, in Engllsh units:

2 Co = 5·12 Lo (^ 4b)

Since the relationship between length, period and velocity of all periodic wave phenomena is defined by: L = CT (5)

COASTAL ENGINEERING

The horizontal and vertical displacements from its mean posltion, a distance z (measured negatively downward) below the still-water surface, are: cosh cos 2IT(x/L - tiT) sinh

~ = iH sinh 2~(d + z)/L sin 2rr(x/L - tiT) (9b) sinh 27Td!L

From these equations it can be seen that the semi-orbital amplitudes of the sub- surface particle's motions are:

a' = cosh^ 2~(d^ +^ z)/L sinh 27Td/L

b' = iH sinh 2;(d + z)/L sinh 27"d/L

with the ratio of the orbital amplitudes (Fig. 5) being:

~: = tanh 2JT(d + z)/L

(lOa)

(lOb)

(ll)

Recent experiments (Morison, 1948) have verlfied these equations (Figs. 6

and 7) except that, in addition, there is some mass transport. The full amplitude of the orbital motion at the surface (2a~ and 2b~) may be expressed as:

2a s ' = H coth 2/Td/L

2b S ' = H

(12a)

(12b)

When the equations are converted into their exponential form,it is found that as the water depth approaches infinity:

a'~ tHe~z/L

b'~ iHe 27TZ^ / L

(13a)

(13b)

However, the horizontal and vertical semi-amplitudes approach these limltlng values at different rates with respect to z (Fig 5). So, although the orbital motion near the surfac·e becomes nearly circular In shape very rapidly as the depth of water increases, the orbital paths become flatter and flatter with increasing dis- tance below the surface until, at the bottom, the vertical motion is zero and so the particle moves back and forth with a purely horizontal motion. Only when the water depth becomes "lnfinite" are all the particle paths circular. Fig. 8a shows the vertical amplitude of oscillation for various depths and wave lengths, and Fig. 8b shows the horizontal amplitude of oscillation for various depths and wave lengths.

By differentiating the horizontal and vertical orbltal displacements with re- spect to time, the horizontal and vertical components of the water particle veloci- ties occupying an average position at a distance z below the center of the surface particle (this neglect of second order quantities appears to be allowable) are found to be:

-ll- 1T_H cosh 21T(d + z)/L sin 2JT(x/L

  • H - T- sinh 27Tli!L tiT) (14a)

vz -~-^ -7TH^ sinh^ 27!(d^ +^ z)/L^ cos^ 27T(X/L^ _^ tiT)

  • H - T sinh 27Td/L (14b)

with the average velocities over one-half their cycle being:

(uz)ave. (^) = +^ 2H^ cosh^ 27T(d^ +^ ZlLL T sinh 27Td!L

(15a)

(vzlave. +^ 2H^

sinh 27T( d + z)/L

T sinh 2 7Td/L

(15b)

B

ELEMENTS OF WAVE THEORY

0.9 (^) (SUR ACE) Zld 0.0 V

V V

O.S

~a

/ V^ 1/

~

1// V

/

V (^) V r-/ V (^) V /"

V (^) V

V

0

./" ~

V

V ~Id'-~ ..,,-

/'

V

Zld· 0.

V /

V

lid· -O.S

V

V"Z/d / V

~ I---^ Zld=^ -

(BOT lid

V

V

V

  • -0.

~ -0.

OM) -1.

~ l--

./

V

l---

I---

!--

V

l-

Fig. 6. Photograph of water particle orbits for a wave with 0 0.1 0.2 0.3 0.4 (^) 0.5 the following dimensions. ...d... Lo Fig. 5 o

0.2^ I

.z.. 0. d

f

Vao

a.

0/

rtf

/ ?

O.S

O.B

o 0.2 0. b ,O.S O.B 1. --.o Comparison of the ratios of measured orbit axes with theory for d/L (^) o =0. Fig. 7

~ o.o",,~Tc!.!!!''F!....!!;F~=:t::::~

t.IL 0.2 1---+-

:!!.J 0.4~-,.0'1--+

~ ~ 0.1 1-+---+~~~+7""~""

IIL

BOTTOM 0.2 0.4 0.1 0.1 1. Zb/H

o

Q

o

Y,

8

O.

d = 2.50 feet, H = 0.339 feet, L = 6.42 feet, T • 1 12 seconds and d/Lo = 0.

~

l.-- ~

/

V

v?

THEORY

  • b' ___ 0 1

MEASURED o-b: 0;/^ I^ J^ )I-a I. 0 .02^ .04^ .06^ .08^ .10^ .12^ .14^ .IS b' 0' (^) FEET b. Comparison of measured orbit semi-major and semi-minor axes with theory: d/Lo= 0.

~ til 0.0 If b' J' o. 1/ /

% 0.2 I-- ';'/..'a'?f-l~.~-f--lJr-+-++--+-~++-...u~--+---- ~ (^) 0.4 ~ (^) b ./1; .;:: I--?,- "'" ~ .... I-- ~1-1-'''''~''---+--- ;I. J l) ~ ~ ~ " ~ 0.6 J-+--+I+-+-+-+-,J---j--+-I--+--I-----j~___j

UN 'ST RA~r

~ ~ ~ 0.8 H--H+--+-+--+-JH----+-I z~· • coshTCd+Z) f '1 .i~~ ~I 1.0 '-L--'--1-'------'----'---.L.J...B"'OT'-'T""01l"-.J....l...--.J^1 L-1L-^11 ---.JL- ° 1.0 2.0 3.0 4.0 5. Za"H RATIO OF VERTICAL AMPLITUDE OF ORBIT TO WAVE HEIGHT RATIO OF HORIZONTAL AMPLITUDE OF ORBIT TO WAVE HEIGHT a. Vertical amplitude of oscillation for proportional depth related to fraction of wave height.

b. Horizontal amplitude of oscillation for proportional depth related to fraction of wave height.

Fig. 8

0: ::> o '"

o 3

o Z

o I

2 I 0

~ 0 ~ 0 ~ 0 III 0 0: ~ G ti... ... 0

7

5 4

I 0 o

ELEMENTS OF WAVE THEORY

MAXIMUM VELOCITY OF WATER PARTICLES ON THE OCEAN BOTTOM FOR VARIOUS DEPTHS AND PERIODS THE ORDINATE IS THE VELOCITY DIVIDED BY THE WAVE HEIGHT THESE CURVES ARE FOR

-H-::'T1,nhT^ (u.l^ .....^ x^ 1r^ (2TTd)

,\

~ ~ \

""

-:::::::: (^) t---t-- 1~5 ............^ ~ -:--t----^ -IS^

T-2e (^) SEC (^100 200 400 500 600 700 800 ) DEPTH OF WATER I FEET

Fig. 9

/

V^1000 • $^ Lfl^^2 84 HOURS /

/ /

WHEN L IS IN FEET

./

800

.,^600 0: ::> (^0 ) '"; /

V

/


V

ZOO

OZ 04 06 OB 10 10 ZO 30 WAVE LENGTH, FEET WAVE LENGTH, FEET 00 (~

/

/

40

Relationship between modulus of decay due to viscous damping and wave length.

." "- '" Z 0- IL '"^0 ..J '"Z 0 i=II: IL^0 II:^0 IL

00

02

04

06

08

o

I

Fig. 10

I J--

r- ...--....- 095 ~~ (^) ~ -- --

--

..-- / (^090) /" -

I

080 /" ~

j (^070) / ~ - II (^) II (^) V 016t -- /'

./

....- ~

I /^ I

050 /' /

/ (^0 40) L

I II^ II^

V (^) / ;3<: / II I I / /

;

I I (^) I I

II I

01 02 03

I

I

04 d/L

o{

/

I 05

SURFACE

~ f..--- ~^ f.--^ -^ f..--- --

f--

V ~

--

~

f--

V-

V

l-- ,./'

V

./ V K= 'Qlh 211 (I+Zldlll. cosh 211d/L where I • DISTANCE BELOW SURFAa d • DEPTH OF WATER L • WAVE (^) LENGTH

BOTTbM (^06 07 )

Fig. 11. Pressure response factor.

50

COASTAL ENGINEERING

as engineering applications are concerned, for waves of appreciable height. It has

also been observed that the very long, low ocean swell from distant storms are ap-

proximately sinusoidal in deep-water. However, for waves of greater height, theory

indicates that certain corrections are necessary.

Two theories have been developed for waves of finite height. The first

theory, developed by Gerstner (1802) and later by Froude (1862) and Rankine (1863),

is known as the trochoidal theory. This theory has been used widely by naval

architects and engineers in their studies. The second theory, developed princi-

pally by Stokes (1847) and later by Struik (1926) and Levi-Civita (1925), is more

difficult to apply but it predicts certain results that have been experimentally

verified which are not predicted by the trochoidal theory.

Trochoidal Theory - Infinite Water Depth. Tne trochoidal theory (Gerstner, 1802),

the first theory to be developed for waves of finite height, is often used for

engineering calculations. One reason for its use is the ease with which the equa-

tions may be used. It appears to represent the actual wave profiles as well as

actually satisfying the pressure conditions at the surface and the continuity con-

ditions. However, it requires rotation of the particles and does not predlct any

mass transport in the direction of wave propagation, while observations (Mitchim,

1940; Beach Erosion Board, 1941) show that there is mass transport. This theory,

developed for waves in water of infinite depth, has been well presented by Gail-

lard (1935).

The equations of the surface profile (Fig. 12a) are,

x = Re - r sin e

y = R - r cos e

(22a)

(22b)

It can be seen that the wave length, La, is equal to 2ffR, while the wave height,

Ho, is equal to 2rs, where rs is the value of r for the surface orbit. In order to

plot the equation of wave shape in dimensionless form with the origin of the coor-

dinates at the crest and the vertical dimension measured negatively, downward,

these equations may be transformed to:

x'/L (^) O = 1 - [(rad e/2~) - (H (^) o/2L (^) o )sin6]

y'/H (^) o = 1/2(1 - cose)

(22c)

(22d)

where, x' and y' are measured from the wave crest. These have been plotted in

Fig. 13 with Ho/Lo as the parameter. It can be seen that as Ho/Lo approaches zero,

the curve approaches a sine wave and the surface is nearly that as developed in the

irrotational theory for waves of very small amplitude.

are,

The positions of the crest and trough relative to the undisturbed water level

Height of crest = Ho - [rs - (rs2/2R)] = 1/2Ho +rrHo2/4Lo

Depth of trough = 2"R[r (^) s - (rs2/2R)]/Lo = 1/2Ho - rrHo2/4Lo

(23a)

(23b)

Thus, the crest is more than half the wave height above the undisturbed water

level, while the trough is less than half the wave height below this level. Ex-

periments performed by the Beach Erosion Board (1941) verify these relationships

(Fig. 14). It should be noted that they verify the results of the theory of

Stokes (1847) as well.

The paths described by the water particles during one cycle are circles with

the radii decreasing exponentially with depth (Fig. 12b). This is expressed as,

a' - b' - r e2~z/Lo - 1/2H e 2"z/Lo

    • s - 0 (24)

COASTAL ENGINEERING

The energy of the wave is equally divided between kinetic and potential, with

the total energy being,

Trochoidal Theory - Finite Depth. The trochoidal theory as extended to water of

finite depth has been presented by Gaillard (1935) and is widely used. There ap-

pears to be no published mathematical work which substantiates the conclusions pre-

sented by Gaillard (1935). Perhaps the facts that (a) the wave velocity, orbital

velocities and wave shapes as represented in the trochoidal theory were the same as

those in the theory of Airy (1845) for waves in deep-water, and (b) other equations

of the trochoidal theory reduced to those of Airy (1845) for small amplitudes led

Gaillard (1935) to examine the similarities b0tween equations from a reduced (el-

liptical) trochoidal theory and the Airy (1845) theory for waves in finite depth.

The equations of wave velocity, and orbital velocities and shapes as obtained from

the reduced trochoidal theory are the same as those of Airy (1845) for shallow-

water waves and for small amplitudes. Other reduced trochoidal equations are al-

most identical to those of Airy (1845). However, the reduced tr choid theory does

not satisfy either the conditions of continuity or dynamical equilibrium except at

the trough and crest (Gaillard, 1935) and hence, this theory, although widely used,

is not sound.

Gaillard (1935) states that a shallow-water wave differs from a wave in very

deep water in that the particle paths are elliptical rather than circular, with

the eccentricity of the ellipses depending upon the ratio of the wave length to

the depth of water. For a particular length of wave, the eccentricity increases

with decreasing water depth so that, in very shallow water, its particle paths are

nearly horizontal lines; while the orbits decr~ase in size with increasing dis-

tance below the undisturbed water level with the vertical axes decreaSing at a more

rapid rate than the horizontal axes until, at the bottom, the vertical motion is

zero and the particle moves in a horizontal line. The angular velocity is not con-

stant, but greatest in the vicinity of the trough and crest. It should be noted

that this theory predicts that the velocity at the crest of the orbit is the same

as the velocity at the bottom of the orbit. Recent experiments performed in the

wave channel at the UniverSity of California, Berkeley, show that this is not true.

The actual crest velocities are greater than the trough velocities.

The following equations, describing the reduced trochoidal surface, were de-

veloped and presented by Gaillard (1935) (Fig. 15),

x = Re - a'sine

y = b'cose

The velocity of propagation is,

C2 = gLb (^) s '/2rra (^) s ' = gL(tanh ~d/L)/2~

The equations for the semi-axes of the orbits are,

b' = 1/2H[cosh 2~(d + z)/L]/sinh 2ffd/L

a' = 1/2H[sinh ~(d + z)/L]/sinh 2~d/L

and the ratio of the semi-axes is,

b' a' =^

tanh 2~(d + z)/L

(26a)

(26b)

(lOa)

(lOb)

(ll)

The total energy of the wave, which is one-half kinetic and one-half potential, is

E (27)

where M, the energy coefficient, is

M = 7r 2/(2 tanh 2 2;>rd/L) (28)

ELEMENTS OF WAVE THEORY

y

~o~~____~____~~~____________-,X

a

Fig. 15. Shallow water wave, trochoidal theory.

The equations for the shape of the surface profile may be wrltten in a dimension-

less form,

x/L = [rad(arc cos 2y/H)/2ff]-[H sin(arc cos 2y/H)/2tanh 2ffd/L] (29)

This, together with the equation for the displacement of the crest and trough from

the undisturbed water level (Yswl)'

Yswl/H = 1/2 - (1TH/4L)tanh 21Td/L (30)

allows the plotting, in dimensionless form, of the wave profile, or, as x/L = tiT,

the variation of surface elevation with time. Experlments (Wiegel, 1950) have

shown that actual waves are very closely trochoidal in shape (Fig. 16). It should

be pointed out that these profiles (i.e., for these values of d/L) are v~ry nearly

the same as given to the third approximation by Stokes (1847). If the equations

for the trochoid are expanded into a series, it can be seen that to the third term

it is the same as Stokes I equation as well.

Trochoidal Theory - Rotation. Stokes (1847) has shown that the trochoidal theory

necessitates rotation and derives the following expression,

Vorticity = 2w.

YL • 049 'YL • 0 037 '!1. ·0.32 YL • 030. 'Yc.0026 ~. 022

T ·0885Eo. d. 189" T^ ^116 SEC^ d.^2 17 FT^ T • 114SEG d- 189FT T • I 43SEC d -217FT

  • --- - EXPERIMENTAL - - - - EXPERIMENTAL - - -- EXPERIMENTAL - - - - EXPERIMENTAL ----- THEORY (^) ----- THEORY ----- THEORY (^) -- THEORY 06 I I

I

06 I I

_Ll I I

~~

OUtlOTION

r- Of -~r-

~ 'R~N - r-

04

I If" r-~-

DIRECTION ~~

Of

r-H.- PROPAGATION

_Ll

=~

_ DIRECTION

Of^ r-Ir-

-P~N r-f-r-

" I I I"

=

r--- DIRECTION

r- PROPAGATION Of^ r-tt^ -

--+-r-^ -

04

02

~ \ I

1
, (^) II ~O^ \ II.' Utc 1'"- \ /J

~ I

02 rl 1\

I I I), /'^ 0.2 02 0.2 -

i'-.t-

r .... 1-"

I 0.4 (^) ,.-'., 0.4 (^04) 02 04 06 08 10 YT

02 04 06 08 YT

  1. o^ 0.2^ 0.4^06 08

iT

o 02 04 06 08 YT

(0) (^) (b) (e) (^) (d)

Fig. 16. Comparison of experimental elevation-time curves with trocholdal theory.

ELEMENTS OF WAVE THEORY

The equation for the wave profile, to the third approximation, is:

y = a COS2~/L+(~a2/L)(cos4rrx/L)[(e2~d/~e-2rrd/L)(e4rrd/~e-4rrd/L+4)~ +

(e2rrd!L_e-21Od!L)

2 3/2 ( 6 / (e12rrd/L+e-12rrd/L)+14(eSrrd/L+e-S~d/L)+19(e4~d/L+e-4~d/L)+32]

rr a L) cos TrX L)[ 6-

(e2~d/L_e-2~d/L) (34)

The equations for the horizontal and vertical components of orbital velocities

are (according to verbal communication from R. A. Fuchs, Institute of Engineering

Research, University of California, Berkeley).

d? _ ~.C [COSh2~(d + z + '1! )/L] cos[2lr(x +f _ Ct)/L] +

dt L sinh2~7L

3(TH~ 2 C [cosh4'1r(d + z -" )/L] cos[4 ..... (x + " 4 L' l (sinh2~d/L)4 > - Ct)/L] (35a)

which, upon expanding, substituting and neglecting terms of third order or higher,

becomes,

C

(sinh2"'d!L)

II

1 3 cosh L (d+z)

[-2 + 4 (sinh2'J1"d/L)2] cos (35b)

and,

E-'I! = 'JI"H ·C [sinh2lr{d+z+ 7J )/L] ( i 2 ( J-Ct)/L)-

dt L sinh2lrd!L J s n T x+

3 'lrH 2 sinh41r( d+z+ 'Ij )

1+ (1:) c [(Sinh2...-d/L)4 ] (sin4T(x+ f -Ct)/L) (35c)

which, upon expanding, substituting and neglecting terms of third order or higher,

becomes,

d 11 '/rH sinh2lr(d+z)/L 3 'JI"H 2 sinh4T(d+z)/L

dt =L· Csinh2'11tl/L (sin2"1T'(x-ct)/L)-4tL"J cf (sinh2'1rd/L)4Hsin41r(x-Ct)/L) (35d)

The equations for particle displacement about their undisturbed positions are,

f :!!. cosh2'!r(d+z)/L ( i 2'-' Ct)/L)

2 sinh2~7L s n "\x- -

'lrH2 [ 1 3 cosh4'1r(d+z)/L lrH 2C COSh4lr(d+Z)/L. t

4L(sinh2~d/L)2 -2+4 (sinh2'11tl/L)2 ](sin4'J1"(x-ct)/L)+(~)·2· (sinh2~d/L)2 (36a)

and,

Thus, the particle orbit lies a little above an ellipse at the crest and is a

little flatter than an ellipse at the trough while, at the same time, the particle

is moving forward (i.e., mass transport). This is shown in Fig. lS.

These equations show the most interesting result of the theory of Stokes

(1847). That is, by not neglecting the effect of height (the velocity of a par-

ticle depends not only upon its mean position, but also upon its displacement from

its mean position) it is shown that the particle velocity is greater in its forward

COASTAL ENGINEERING

CREST

-.


r-.... d'^2 OOOFT

/

~

T' 2 000 SEC H' 0.400 FT Z ' 0 (SURFACE PARTICLE)

~L'1440 FT

C' 7 198 FTISEC

J

I \

UNDISTURBED WATER SURFACE

I/X,y


j

""

~

~

v


  • 20 r^ MASS TRANSPORT ~ .. 40 .. (^30) ... 20 .. (^10) o - 10 -.20 - 30

" FEET Fig. 18 Theoretical orbit of surface particle - Stokes' irrotational theory, second order.

movement (with the crest) than in its backward movement (with the trough). Labo- ratory experiments performed at the University of California, Berkeley, confirm this conclusion. This results in the fact that the forward motions of the par- ticles are not altogether compensated by their backward motions. Hence, in addi- tion to their orbital motion, there is a progressive motion in the direction of propagation of the waves. The orbits are open, not closed (Figs. 6 and 18). This motion has become known as "mass transport" and is given to the second approxima- tion by

07a)

For deep-water, this becomes,

00 = (~Ho/Lo)2 Coe4~z/L (^) (37b)

which is identical with the equation expressing the horizontal velocity remaining (due to rotation) after wave motion has been destroyed ln the rotational trochoidal theory (Equation 31). In other words, in order for a wave of finite height to exist, it is necessary for this additional velocity to exist. In the trochoidal theory, it is in the form of molecular rotation (which is not substantiated by ob- servations) of particles moving ln a closed orbit, while, in the irrotational theory, it results from particles moving in an open orbit (which is substantiated by observations (Beach Erosion Board, 1941; Mitchim, 1940; Morison, 1948).

Maximum Theoretical Wave Steepness. Stokes (1847) came to the conclusion that for any wave whose crest angle was greater than 120 0 , the series would cease to be con- vergent and hence the wave form would become discontinuous. However, the possibil- ity of a wave existing with a crest angle equal to 120 0 was not shown until later. Michell (1893) found the theoretlcal limit was H/L - 0.14 and Havelock (1918) found it to be 0.1418.

COASTAL ENGINEERING

Folsom, R.G. (1947). Sub-surface pressures due to oscillatory waves: Trans. Amer. Geophys. Union, vol. 28, pp. 875-881.

Folsom, R.G. (1949). Measurement of ocean waves: Trans. Amer. Geophys. Union, vol. 30, pp. 691-699.

Froude, W. (1862). On the rolling of ships: Trans. Institute of Naval Architects, vol. 3, pp. 45-62.

Gaillard, D.D. (1935). Wave action in relation to engineering structures: Re-

printed at the Engineer School, Fort Belvoir, Virginia.

Gerstner, F. (1802). Theorie der wellen: Abhandlungen der Koniglichen Bohmischen

Gesellschaft der Wissenschaften, Prague; also, Gilbert's - Annalen der Physik,

vol. 32, pp. 412-445.

Havelock, E.T. (1918). Periodic irrotational waves of finite height: Proc. Royal Soc., London, Series A, vol. 95, pp. 38-51.

Hough, S.S. (1896). On the influence of viscosity on waves and currents: Proc., London Mathematical Society (1), vol. XXVIII, pp. 264-288.

Isaacs, J.D. and Wiegel, R.L. (1950). The thermopile wave meter: Trans. Amer. Geophys. Union, vol. 31, pp. 711-716.

Kaplan, K. (1950). Idealized model studies of the motion of surface waves: Tech. Report HE 116-316, Institute of Engineering Research, University of Cali-

fornia; Berkeley, California, (unpublished).

Lamb, H. (1932). Hydrodynamics, Sixth Edition, Cambridge Univ. Press.

La Place, P.S. (1775-76). Recherches sur quelques points du systeme du monde: Mem. Ac. Royal Soc., pp. 542-551.

Levi-Civita, T. (1925). Determination rigoureuse des ondes d'ampleur finie: Math. Annalen, vol. 93, pp. 264-314.

Manning, G.C. (1939). The motion of ships among waves: Principles of Naval Archi-

tecture, vol. II, Edited by Tossell and Chapman.

Michell, J.H. (1893). On the highest waves in water: Philosophical Magazlne, (5), vol. XXXVI, pp. 430-437.

Mitchim, C.F. (1940). Oscillatory waves in deep water: The Military Engineer, vol. 32, pp. 107-109.

Morison, J.R. (1948). Wave pressures on structures: Master of Science thesis in

Engineering, University of California, Berkeley, California, (unpublished).

Morison, J.R. (1951). The effect of wave steepness on wave velocity: Trans. Amer. Geophys. Union, vol. 32, pp. 201-206.

Rankine, W.J.M. (1863). On the exact form of waves near the surface of deep water: Philosophical Transactions of the Royal Society, London, pp. 127-138.

Rayleigh, Lord (1877). On progressive waves: Proc., London Mathematical Society, vol. IX, pp. 21-26.

Reynolds, O. (1877). On the rate of progression of groups of waves and the rate at which energy is transmitted by waves: Nature, vol. 16, pp. 343-344.

ELEMENTS OF WAVE THEORY

stokes, G.G. (1847). On the theory of oscillatory waves: Trans., Cambridge Philo-

sophical Society, vol. VIII, p. 441, and Supplement Scientific Papers, vol. I,

p. 314.

Struik, D.J. (1926). Determination rigoureuse des ondes irrotationeles periodiques

dans un canal a profondeur finie: Math. Annalen, vol. 95, pp. 595-634.

Wiegel, R.L. (1948). Oscillatory waves: Bulletin of the Beach Erosion Board,

Special Issue No.1, Corps of Engineers, Washington, D.C.

Wiegel, R.L. (1950). Experimental study of surface waves in shoaling water:

Trans. Amer. Geophys. Union, vol. 31, pp. 377-385.