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Chap 2. Statistical Properties and Spectra of Sea Waves

2.1 Random Wave Profiles and Definitions of Representative waves

2.1.1 Spatial Surface Forms of Sea Waves

 Long-crested waves: Wave crests have a long extent (swell, especially in shallow water)

 Short-crested waves: Wave crests do not have a long extent, but instead consists of short segments (wind waves in deep water)

2.1.2 Definition of Representative Wave Parameters In nature, no sinusoidal wave exists

→ Wave forms are irregular (or random)

→ Difficult to define individual waves

→ Zero-crossing method is used.

(2)

Assume that we measured (t) at a point.

Zero-upcrossing:

Zero-downcrossing:

Statistically, zero-upcrossing and zero-downcrossing are equivalent if the wave record is long enough. But zero-upcrossing is more commonly used.

(3)

Arrange the wave heights in descending order.

(a) Highest wave: Hmax, Tmax

Note: Tmax is not the maximum wave period in the record, but the wave period corresponding to Hmax.

(b) Highest one-tenth wave: H1/10, T1/10 Average of the highest N/10 waves

/10

1 10

/

1 /10

1 N

i

Hi

H N

10 /

T1 = average of the wave periods corresponding to the highest N/10 waves (c) Significant wave, or highest one-third wave: H1/3, T1/3 (or Hs, Ts)

/3

1 3

/

1 /3

1 N

i

Hi

H N

(d) Mean wave: H (or H1), T

N

i

Hi

H N

1

1

(4)

2.2 Distribution of Individual Wave Heights and Periods

2.2.1 Wave Height Distribution

Gaussian stochastic (linear) theory for narrow-band spectra (range of periods is small) suggests Rayleigh distribution of Hi (discrete) = H (continuous) for large N. Probability density function:



 



2

exp 4 ) 2

(x x x

p  

with H xH

satisfying ( ) 1

0

p x dx

Probability of exceedance:

) given

~ (arbitrary~ y

probabilit

exp 4 exp 4

) 2

( 2 2

H x x H

x d

x

P x



 



 

 



Field data indicate that Rayleigh distribution based on restricted assumptions (linear + narrow-band) yields good agreement with data.

(5)

2.2.2 Relations between Representative Wave Heights Exceedance probability based on Rayleigh distribution

x N x

P N N 1

exp 4 )

( 2 

 



 

2 /

)1

2 (ln N xN

  for given N (e.g., N = 3, 10) By definition

 

N N

N

x x

N x

N xp x dx

dx N x p

dx x xp H

x H ( )

/ 1

1 )

( ) (

/ 1 /

1

Using p(x) dx

dP  and P x x

x pd ) 4 (

exp )

( 2

 

 





 

 





 





 



N N

N N N

N x N

N x N

x x N x

dx x x

x N

Pdx x

P x N

dx P xP

N

dx dx xdP N

x

2 2

/ 1

exp 4 exp 4

) (

) ( ]

[

using complementary error function,

x  t dt e

x) 2

(

erfc ,



N N

xN

N N x x t dt

x

2

2 2

/ 1

) 2 4 exp(

exp

N N

N x N x

x 2 erfc 2

/ 1

 with 2 (ln )1/2

N xN

(6)

See Table 10.1 (p 373) for H1/N /H vs N100,50,20,10,

H H

Hs1/3 1.6 , H1/10 1.27Hs, H1/100 1.67Hs

2.2.3 Distribution of Wave Periods Not well established.

Local wind waves (~10 s) + Swell (~15 s) → two peaks (bi-modal) or two main direction Typically, TmaxT1/10T1/3 (1.1~1.3)T

2.3 Spectra of Sea Waves

2.3.1 Frequency Spectra

Free surface oscillation at a point:

1

) 2

cos(

) (

n

n n

n f t

a

t  

where

an = amplitude of wave with frequency

n

n T

f 1

n = phase of wave with frequency fn

(7)

Energy of wave with frequency fn = 2 2 1

gan

Real sea waves → infinite number of frequency components → (continuous) frequency spectrum

Note: anS(fn)f 2

1 2

an  2S(fn)f

(8)

Standard spectra

ensemble average of large number of wave records (1) Bretschneider-Mitsuyasu spectrum

Fully developed wind waves in deep water

(energy input from wind = energy dissipation due to breaking)

] ) ( 03 . 1 exp[

257 . 0 )

(fH2T4f 5T f 4

S s s s (2.10)

for given Hs and Ts.

Modified by Goda (1988): 0.257→0.205, 1.03→0.75 as in Eq. (2.11).

(2) JONSWAP (JOint North Sea WAve Project) spectrum Growing wind seas in deep water

] 2 / ) 1 ( 4 exp[

5 4

2 2 2

] ) ( 25 . 1 exp[

)

(f  JHsTp f Tpf Tpf S

where

) (

JJ (2.13) )

, ( s

p

p T T

T  (2.14)



 

p b

p a

f f

f f for 09 . 0

for 07 . 0

 

peak enhancement factor  1~7 (typically 3.3)

Need to specify Hs, Ts, a, b, and  (sharper spectral peak as  ↑).

(9)

Suh et al. (2010, Coastal Engineering 57, 375-384) showed that for deepwater waves around the Korean Peninsula, the probability density function of  is given by a lognormal distribution:











 

2

53 . 0

58 . 0 ln 2 exp 1 2

53 . 0 ) 1

( 

  p

with its mean equal to 2.14, which is somewhat smaller than 3.3 in the North Sea.

0 1 2 3 4 5 6 7 8 9 10

g 0

40 80 120 160

Number of g

0.2 0.4 0.6 0.8

ProbabilityDensity

Histogram

Lognormal PDF(m=0.63, s=0.51)

(10)

(3) TMA spectrum (Bouws et al., 1985, J. Geophys. Res., 90, C1) ↓

Includes effects of finite water depth )

, (f h S

STMAJk

Kitaigordskii shape function (depth effect)





2 for

1

2 1

for ) 2 ( 5 . 0 1

1 for 5

. 0 )

,

( 2

2

h h h

h h

k f h

2 /

)1

/ ( 2 f h g

h

 

(11)

2.3.2 Directional Wave Spectra (1) General

frequency spectrum → assumes waves with many different frequencies but single direction.

However, real sea waves consist of many component waves with different frequency and different direction. Therefore, we need directional wave spectrum:

( , ) ( ) ( | ) S f  S f Gf

directional spreading function ↓

directional distribution of wave energy ↓

varies with frequency f .

( | ) 1

G f d

 

 

represents relative magnitude of directional spreading of wave energy

∴ Total energy =

 

0 S(f, )d df

 

=

0 S f G( ) ( | )f d df

 

 

=

0S(f)df

(12)

(2) Mitsutasu-type directional spreading function Based on field measurements,

2

( | ) 0cos 2 GfG s  

  ← symmetric about  0

 = wave angle from principal direction ( 0) See Fig. 2.11 for the variation of G versus .

Intuitively, G0 for 180 90 and 90 180. But, G is very small as long as s is large.

Must satisfy 1

cos2 2

0  

 

 

d

G s

Symmetric about  0: 1

cos 2

2 0

2

0  

 

d

G s

) 1 2 (

)]

1 ( 2 [

1 cos 2

2

1 2 1 2

0 2

0  

 



 

 

s

s d

G s

s   

where Gamma function (n)(n1)! for integer n.

(13)

s depends on frequency f :



p p

p p

f f f

f s

f f f

f s s

for )

/ (

for ) / (

5 . 2 max

5 max

where

p

p T

f  1 = peak frequency, and roughly Tp 1.05Ts.

smax

s at ffp, and s decreases as ffp increases.

Hence, directional spreading is the narrowest near ffp. See Fig. 2.12 for smax 20 where f* f / fp (=1 at peak frequency).

(3) Estimation of the spreading parameter smax As smax increases, more long-crested.

Tentatively,





swell for 75

~ 25

waves for wind 10

max max

s

s in deep water.

smax increases as H0/L0 decreases (see Fig. 2.13).

However, Suh et al. (2010, Coastal Engineering 57, 375-384) showed that for wind waves of 0.03H0/L00.055, the mean value of measured smax is somewhat greater than that in Fig. 2.13.

(14)

0.005 0.01 0.02 0.05 H0/L0

1 10 100

2 5 20 50 200

Spreading Parameter, Smax

They also showed that the probability density function of smax is given by a lognormal function:











 

2 max

max

max 0.61

13 . 3 ) ln(

2 exp 1 2

61 . 0 ) 1

( s

s s

p

0 10 20 30 40 50 60 70 80 90 100 110 120

smax 0

40 80 120

Number of smax

0.04 0.08 0.12 0.16

Probability Density

Histogram

Lognormal PDF(m=3.13, s=0.61)

(15)

As waves propagate to shallow water, they become long-crested due to refraction. In other words, smax increases as h decreases. On the other hand, smax increases more rapidly with decreasing h for a larger incident angle because of more refraction (see Fig. 2.14).

(4) Cumulative distribution curve of wave energy Read text.

(5) Other directional spreading functions Simplest:

2

0 0

0

2 !! cos ( ) for

(2 1)!! 2

( | ) ( )

0 for

2 l l

G f G l

    

  

  

   

 

  

  



(2.30)

which is independent of f .

SWOP (Stereo Wave Observation Project):

( | ) ( | )

GfG   ;  2f (2.31) Eq. (2.30) with l1 and (2.31) are similar to Mitsuyasu-type with smax 10, though the energy spread with f is not the same.

Wrapped normal function (Borgman, 1984):

2

0 1

( )

1 1

( | ) exp cos ( )

2 2

N

n

Gf n n 

 

 

    

 

0 = mean wave direction

= directional spreading parameter (broad directional spreading as  )

(16)

2.4 Relationship between Wave Spectra and Characteristic Wave Dimensions



domain frequency

spectrum Wave

domain time

analysis wave

- by -

Wave ← relates each other.

1

) 2

cos(

) (

n

n n

n f t

a

t  

2

1

2 cos(2 )

 

 

n

n n

n f t

a  

 

T

n

n n

n f t dt

T 0 a

2

1

2 1 cos(2  )

Using orthogonality, 1 cos( )cos( ) 0

0

T m t n t dt

T   if mn,

0 0 1

2

0 1

2 2 2

) ( 2 1

) 2

( 1 cos

m df f S

a

dt t

f T a

n n T

n

n n n



 

 

 

where m0 = zeroth moment of S(f)

2 = variance of (t)

Defining rms  2 = root-mean-squared value of (t), we get

0

2 m

rms   

For Rayleigh distribution of H,

(17)

4 0

4 m

Hs  rms

Since Hs and 4 m0 are not exactly the same, use

3 /

H1

Hs  = average height of highest 1/3 waves from zero-crossing method

0

0 4 m

Hm  = spectral estimate of significant wave height

As for wave periods,

p

s T

T 0.95

2 0/m m

T  ;

0 2

2 f S(f)df

m = 2nd moment of S(f)

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