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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
R. L. WIegel and J. W Johnson Respectively, Institute of Engineermg Research, and DiviSlOn of MechanIcal Engmeering UmversIty of Callforma Berkeley, Callforma
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,
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.
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.
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:
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
1'-" l 'II I' , f f
~PE CEN^ DIFFERENPE / c!. 9 Lo^ .~^ ,/
~ 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=
~
'~+ ~~'"
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
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)
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)
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:
(12a)
(12b)
When the equations are converted into their exponential form,it is found that as the water depth approaches infinity:
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:
with the average velocities over one-half their cycle being:
(uz)ave. (^) = +^ 2H^ cosh^ 27T(d^ +^ ZlLL T sinh 27Td!L
(15a)
T sinh 2 7Td/L
(15b)
0.9 (^) (SUR ACE) Zld 0.0 V
V V
O.S
~
/
V (^) V r-/ V (^) V /"
V (^) V
V
0
./" ~
V
V ~Id'-~ ..,,-
/'
Zld· 0.
V /
V
lid· -O.S
V
V"Z/d / V
(BOT lid
V
V
V
~ -0.
OM) -1.
~ l--
./
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
.z.. 0. d
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---+-
~ ~ 0.1 1-+---+~~~+7""~""
BOTTOM 0.2 0.4 0.1 0.1 1. Zb/H
o
Q
o
8
O.
d = 2.50 feet, H = 0.339 feet, L = 6.42 feet, T • 1 12 seconds and d/Lo = 0.
~
l.-- ~
/
V
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.
% 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.
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
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
,\
~ ~ \
""
-:::::::: (^) t---t-- 1~5 ............^ ~ -:--t----^ -IS^
T-2e (^) SEC (^100 200 400 500 600 700 800 ) DEPTH OF WATER I FEET
/
V^1000 • $^ Lfl^^2 84 HOURS /
/ /
WHEN L IS IN FEET
./
800
.,^600 0: ::> (^0 ) '"; /
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
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
04 d/L
o{
/
I 05
SURFACE
~ f..--- ~^ f.--^ -^ f..--- --
V ~
--
~
V-
l-- ,./'
./ 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
x = Re - r sin e
y = R - r cos e
It can be seen that the wave length, La, is equal to 2ffR, while the wave height,
x'/L (^) O = 1 - [(rad e/2~) - (H (^) o/2L (^) o )sin6]
y'/H (^) o = 1/2(1 - cose)
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
x = Re - a'sine
C2 = gLb (^) s '/2rra (^) s ' = gL(tanh ~d/L)/2~
b' a' =^
M = 7r 2/(2 tanh 2 2;>rd/L) (28)
y
~o~~____~____~~~____________-,X
a
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,
T ·0885Eo. d. 189" T^ •^116 SEC^ d.^2 17 FT^ T • 114SEG d- 189FT T • I 43SEC d -217FT
I
06 I I
_Ll I I
~~
OUtlOTION
04
I If" r-~-
DIRECTION ~~
Of
_Ll
=~
_ DIRECTION
=
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
o 02 04 06 08 YT
(0) (^) (b) (e) (^) (d)
y = a COS2~/L+(~a2/L)(cos4rrx/L)[(e2~d/~e-2rrd/L)(e4rrd/~e-4rrd/L+4)~ +
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]
3(TH~ 2 C [cosh4'1r(d + z -" )/L] cos[4 ..... (x + " 4 L' l (sinh2~d/L)4 > - Ct)/L] (35a)
C
[-2 + 4 (sinh2'J1"d/L)2] cos (35b)
E-'I! = 'JI"H ·C [sinh2lr{d+z+ 7J )/L] ( i 2 ( J-Ct)/L)-
1+ (1:) c [(Sinh2...-d/L)4 ] (sin4T(x+ f -Ct)/L) (35c)
dt =L· Csinh2'11tl/L (sin2"1T'(x-ct)/L)-4tL"J cf (sinh2'1rd/L)4Hsin41r(x-Ct)/L) (35d)
f :!!. cosh2'!r(d+z)/L ( i 2'-' Ct)/L)
4L(sinh2~d/L)2 -2+4 (sinh2'11tl/L)2 ](sin4'J1"(x-ct)/L)+(~)·2· (sinh2~d/L)2 (36a)
CREST
-.
/
~
T' 2 000 SEC H' 0.400 FT Z ' 0 (SURFACE PARTICLE)
C' 7 198 FTISEC
I \
UNDISTURBED WATER SURFACE
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
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.
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-
Gerstner, F. (1802). Theorie der wellen: Abhandlungen der Koniglichen Bohmischen
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-
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-
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
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.