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Figure 7.3 Mean power spectrum of incipient-breaking (solid line) and post-breaking (dashed line)
waves. 95% confidence limits are shown. Figure is reproduced from Young & Babanin ( 2006a )
© American Meteorological Society. Reprinted with permission
Confidence limits are very small, and overall the spectra of broken waves lie below the
95% confidence limits of the spectra of non-breaking waves. The higher-order moments
also exhibit interesting substantial differences:
S k i
=
0
.
45
,
S k p =
0
.
31
,
A s i
=−
0
.
186
,
(7.15)
A s p =−
0
.
017
,
=
.
,
K i
3
34
K p =
2
.
96
.
Here, K i and K p are, respectively, incipient-breaking and post-breaking kurtosis
m 4
m 0 .
=
K
(7.16)
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