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GUIDE WAVE ANALYSIS AND FORECASTING - WMO

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108<br />

where: γ = Euler’s constant ≈ 0.5772, and π 2 =<br />

(3.14159) 2 ≈ 9.8696.<br />

For a data set h i (i = 1, ... n), the estimates of popu-<br />

lation mean and variance, – h and s2 , are given by:<br />

1<br />

h = ∑ hi<br />

n i<br />

(9.10)<br />

2 1<br />

2<br />

s = ∑(<br />

hi– h)<br />

.<br />

n – 1<br />

The moments estimators of A and B, ~ A and ~ B, are<br />

obtained from Equations 9.9 and 9.10, which give:<br />

˜ –<br />

(9.11)<br />

If the individual hi are not available, then the mean and<br />

variance can be estimated from grouped data given in a<br />

histogram or a scatter plot.<br />

The two-parameter log-normal distribution is<br />

readily fitted by this method (see Johnson and Kotz,<br />

1970, for further details). The three-parameter Weibull<br />

distribution can also be fitted by moments, the third<br />

parameter being estimated by comparing the theoretical<br />

and estimated skewness (Johnson and Kotz, l970,<br />

p. 257). In theory, the FT-III could also be fitted<br />

by moments but, in practice, it does not appear to be<br />

done.<br />

The method of maximum likelihood consists of<br />

finding values for the distribution parameters, such as A<br />

and B in the FT-I (Equation 9.5), which maximize the likelihood<br />

that the observed data come from this distribution.<br />

This is probably the most widely used method of estimation<br />

in statistics because it generally gives statistically<br />

optimal estimates for large samples, but the method is<br />

often numerically difficult and time-consuming, even if a<br />

computer is available. For example, for FT-I, the maximum<br />

likelihood estimates, Â and ˆB, are given by:<br />

˜ A = h γB<br />

˜ s<br />

Β ≈ 6 .<br />

π<br />

ˆ – ˆ log exp –<br />

ˆ<br />

exp<br />

ˆ –<br />

–<br />

ˆ<br />

exp –<br />

⎡ ⎛ h ⎞⎤<br />

A = B ⎢ ∑ ⎝ B ⎠<br />

⎥<br />

⎣<br />

⎦<br />

h<br />

h<br />

B<br />

B = ∑ h<br />

.<br />

h<br />

Bˆ<br />

∑<br />

1<br />

i<br />

e<br />

n i<br />

i<br />

i<br />

1 i<br />

i<br />

n i<br />

i ∑<br />

i<br />

(9.12)<br />

These equations have to be solved numerically.<br />

The two-parameter log-normal and the twoparameter<br />

Weibull are readily fitted by maximum likelihood<br />

— also requiring numerical solution of equations<br />

— but problems can arise when used for the threeparameter<br />

Weibull (and the three-parameter log-normal).<br />

(See Johnson and Kotz, 1970, for details.)<br />

Both the method of moments and the maximum<br />

likelihood method assume data are statistically<br />

independent and identically distributed. Neither assumption<br />

applies to wave data but the methods appear to be<br />

robust and to give useful results. To meet more nearly<br />

the requirement for independent data, it might be prefer-<br />

i<br />

<strong>GUIDE</strong> TO <strong>WAVE</strong> <strong>ANALYSIS</strong> <strong>AND</strong> <strong>FORECASTING</strong><br />

able to fit data recorded at, say, 24-hour intervals — thus<br />

obtaining separate estimates from all the midnight<br />

values, another from all the 03.00 values, etc. — but this<br />

is not usually done in practice. The considerable annual<br />

cycle in wave height found in many parts of the world<br />

means that the data are often not identically distributed.<br />

As already mentioned in Section 9.4.1.2, it would be<br />

more satisfactory to remove this cycle before carrying<br />

out any statistical analysis but this is rarely attempted.<br />

9.4.1.4 Estimating the associated value of T – z<br />

An estimate of the zero-downcrossing or zeroupcrossing<br />

wave period, T – z, at the time when the<br />

significant wave height has an extreme value, such as<br />

Hs50, is obtained by assuming a specific value for<br />

significant wave steepness. Often, a value of oneeighteenth<br />

is used, so that T – z is obtained from:<br />

2πHs50 1<br />

= ,<br />

2<br />

gT 18<br />

i.e., using metres and seconds:<br />

z<br />

Tz≈34 . Hs50<br />

.<br />

Measurements indicate that one-eighteenth is<br />

appropriate for open ocean sites, but larger values of<br />

about one-fourteenth apply at sites where waves are<br />

fetch-limited. In practice, a value is often obtained by a<br />

visual inspection and extrapolation of the H s – T – z scatter<br />

plot. These rather crude estimates of T – z are often sufficient,<br />

but if the exact value of T – z is important — for<br />

instance if a structure being designed is sensitive to<br />

small changes in T – z — then a range of values should be<br />

specified. For example, ISSC (1979) recommends a<br />

range from approximately 2.6√H s50 to 3.9√H s50, where<br />

H s50 is in metres. (The precise recommendation is in<br />

terms not of T – z but of the period corresponding to the<br />

spectral peak frequency, which is given as approximately<br />

1.41 T – z.)<br />

9.4.2 Return value of individual wave height<br />

A value for the highest individual wave which might<br />

occur is often obtained from the probability distribution<br />

of the maximum individual wave height during the time<br />

(about 3–6 hours) for which the return value of significant<br />

wave height prevails. The mode — the most likely<br />

value — of this distribution is generally quoted but other<br />

values such as its mean may be used (see Sections 1.3.6<br />

and 9.4.1.4 for the required T – z). Alternatively, a data set<br />

may be obtained, consisting of the most likely highest<br />

wave corresponding to each measurement of significant<br />

wave height, and a return value estimated from this<br />

data set.<br />

Both methods are based upon the assumption that<br />

the highest individual wave, Hmax, occurs during the<br />

time of highest significant wave height. This is not<br />

strictly correct. Hmax will most probably occur during<br />

this time but might occur by chance during a time of<br />

lower significant wave height. Values for the maximum

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