JOURNAL
OF GEOPHYSICAL
Multifractal
ocean
RESEARCH,
VOL. 99, NO. C8, PAGES 16,179-16,196, AUGUST
15, 1994
representation of breaking waves on the
surface
Bryan R. Kerman
AtmosphericEnvironment Service,Canada Centre for Inland Waters, Burlington, Ontario, Canada
Lucie Bernier
Department of Computer Science,McGill University, Montreal, Quebec, Canada
Abstract. It is established
for the first time that the spatialdistributionof breaking
waveson the ocean surfaceis a multifractal process. This result is based on an
analysisof airbornevisibleand near-infraredimageryof the oceansurfaceunder a
limited rangeof wind speedand fetch. A detailedstudy of the optical spectraof the
imagesand the cumulativeprobability structureof the prevalentbackgroundshows
that the lower-intensityreflectiveareasfollow a Rayleighprobability distribution.
By contrast, the higher-intensitypixels associatedwith the scatteredlight from
foam and breaking wavesdemonstratescalingcharacteristicsin both the optical
spectra and the cumulative probability distributions. It is demonstratedthat the
degreeto whichthe whitecapsare singularitieson a dark backgroundis describedby
a Lipschitzexponentc•, whichuniquelytags eachbreakingwave. This identification
process,called "fractal" or "singularityfiltering", leadsto a critical conditionc• =
1 tentatively associatedwith the crossoverfrom active entrainingwhitecapsto
passivelydissipatingfoam. The multifractal representationassociatedwith the
degreeof singularityis simply a restatementthat the imagery is composedof a
continuumof sets,whereeachset consistsof thosebreakingwavesat a particular
phasein their existence.The fractal spectrumof the image abovea thresholdis
shownto be representable
by a fractal generator.Physically,the fractal generator
modelsthe energyexchangein a breakingwavefield as a flux of energyinput from
the atmosphereto the wave field cascadedover scalesof the order of a kilometer to
meters. If the energyflux is further parameterizedin terms of the receivingarea,
an assumptionsimilar to closuretechniquesused in classicalturbulence models, the
empiricalresultssymmetricallyspan Phillips'sbasicargumentsfor the energyflux
terms controlling a wind-driven sea.
Introduction
1963, 1983; Srokosz,1986]assumethat the occurrence
statistics of breaking waves arise from a joint GausKnowledgeof the spatial distribution of breaking sian distribution of wave height and slope. While such
waveson the ocean surfaceis required in a number of models have not been examined for their predictions
applicationsas variedas gastransferand soundgener- of spatial statistics, it has remained for modelers to,
ation at the air-sea interfaceto representsomephysical somewhat arbitrarily, assumea Poissonprobability dis-
or chemicalactivity occurringlocallyin terms of larger tribution [Hollell and Hellmeyer, 1988] when dealing
spaceaverages.While someimportant characteristics with the distribution of soundgeneratedunderwater by
of breakingwavesrelevantto theseapplications,such breaking waves. Such a model is inadequateto explain
as fractional coverage,their numberfor a given image the observedintermittency and "groupiness"of breakarea, or their lifetime, have been studied by many au- ing waves, as discussedbelow. Recently, Huang el al.
thors,mostprincipallyMonahah[1993]and Hollhuisen [1992]haveshownthat the intermittent,randomphase
and Herbets[1986],there is limited experimentalev- of surface gravity waves follows a fractal distribution.
idenceto representtheir spatial geometry[Snyderel They show that rms differencein phase over a time inal., 1983]. Sometheoreticalmodels[Longuel-Higgins,terval At is identical within a scalingoperation to a
differenceover eat, where e is somearbitrary multiple.
Copyright1994 by the AmericanGeophysicalUnion.
Paper number945C00590.
0148-0227/94/945C-00590505.00
It is therefore natural to consider such techniques to
describethe strong nonlinearity and intermittency of a
breaking wave field.
Before introducing the so-calledfractal approach to
brea.kingwaves,it is appropriateto attempt to state in a
16,179
16,180
KERMAN AND BERNIER: MULTIFRACTAL BREAKING WAVES
!
. Ii .
i
Figure 1. (a), Field of breakingwavesobserved
usinga line scanneron boardan aircraftflying at
about500m overthe Bayof Fundy.Fieldof viewabout250m2, resolution
wasabout0.5m,andoptical
wavelength
was0.95/•m. (b), Imagethresholded
to removereflective
Rayleighcomponent.
(c), Imageof
asubsets
(a) 1) identifiedwith nonentraining
(foam)areas.(d), Imageof a subsets,
a < 1, identified
with entraining(breakingwave)areas.
qualitative way what is observedabout breakingwaves, at the locationsof the breaking waves. The localized
even at the risk of stating in some casesthe obvious. nature of thesepeaks,akin to islandsof white light in
classical,globalrepreWhen the field is imaged either by standard photog- a blackbackground,discourage
sentations
such
as
a
Fourier
representation
and suggest
raphy [Rossand Cardone,1974;Smith,1981;Kennedy
andSnyder,1983]or with side-scanning
techniques
from
underneaththe surface[Thorpeand Hall, 1983;Thorpe
andHumphties,1980]or fromthe air (Figurela) [Kerman and Szeto, 1994], severalfeaturesof the spatial
field of breakingwavesare evident.
The first feature of breaking wavesis their distinct
isolated nature: the fact that they are born, mature,
and die almostalwayswithout affectingor beingmodulated by other breaking-waveevents. If a line were
drawn arbitrarily acrossthe imageof Figure l a, the local light densitywouldbe decidedlyintermittent,that
is, almosteverywherenearlyuniform,with narrowpeaks
a local topologyand singularitiesto characterizethe
process.Two basiccharacteristics
of individualwaves,
thelightaccumulated
withinthemandtheirsize,define
a uniquemeasureof the singularity that a breaking
waverepresents
in an otherwise
smoothlyvaryingbackground.
The secondfeature of breakingwaveswhich can be
demonstratedadequatelyby laboratory measurements
[Melvilleand Rapp,1988;Papanicolau
and Raichlen,
1988]istheself-similarity
oftheevolution
process.
Each
breakingwaveappearsto be identicalto everyotherexceptfor sizeand duration. In this evolutionall waves
KERMAN AND BERNIER: MULTIFRACTAL
follow a path from their creationas a bright, energetic,
linear bubbling froth to ultimate dissipationas a contorted patch of foam, albeit at different sizes. Consequently,any breaking wavefield has within it individual
breaking waveswhich can be characterizedbroadly by
two properties' initial turbulent energy and age. The
challengeis to estimate these propertiesfrom imagery.
Of importance to later discussionsis the concept that
within a snapshotof an oceanicfield of breaking waves
lie a number of self-similar identities, each at a particular phase in its lifetime and each at its own transient
energy state.
Another feature of a field of breaking waves is the
nonuniformity of the occurrenceof the waves. They are
not uniformly distributed in space,and their occurrence
is not predictablein time. The reasonsfor the clustering
and intermittency are related in part to the modulation
of wave growth and steepeningwithin a wave group's
envelop[Donelanet ai., 1972]and,webelieve,to the inherent intermittency of the energyexchangedriven by
the atmosphere. A Poissondistribution fails to capture
the essenceof intermittency becauseit assumesa constant densityof eventsin space,a fact clearly violated in
the observations.It is necessaryto work with a relaxed
set of assumptionsin which the density of occurrences
BREAKING WAVES
16,181
equivalentto assumingthat the singular structuresof
all breaking waveswhich are basicto the fractal result
have a single, common property. This result disagrees
with our intuitive sensethat a bright new breakingwave
is not geometricallyand dynamicallysimilar to one dissipating at the foam stage. Evidence for a violation
of such a commonbut restrictive singularstructure was
found in the variation of the apparent fractal dimension
as a function of the level of light thresholdthat one imposed. If the field was truly monofractal, it would not
matter what subset of the field was examined, as only
one singularity property was present at all scales.
As mentioned
in the conclusion of Kerman
and Szeto
[1994],it is necessaryto consideran escalationof conceptual difficulty, that is, that a breaking wave field is
associatedwith a multifractal processrequiring many
or a continuum of fractal dimensionsfor its representation. The multifractal approach has much in common
with numerous other geophysicalprocesses,especially
in atmosphericdynamics[$cherlzerandLovejoy,1991].
What will become clear is that the breaking-waverepresentation provides one of the clearest examples of a
multifractal structure and one perhaps easier to motivate physically.
It was our initial purpose to examine whether the
is itself some function of scale.
process was indeed multifractal. As interesting and
Yet another distinguishingfeature of a breaking wave utilitarian as such results may be, the intriguing quesfield is the size range of eventsfrom the obviouslarge tion posedby Kadanoff [1986] (Fractals-Where'sthe
waveswith dimensionscomparableto the energy-contain-physics?) remained. Accordingly,this paper has reing wavelengthsof the gravity wavefield to weakly en- focused on the basic premisesof a multifractal repretraining ripplets that are barely visible,the so-calledmi- sentation from which has arisen the conceptof singucrobreakers
[PhillipsandBanner,1974].Phillips[1985] larity filtering to isolate individual breaking wavesand
has argued that there exists within the wave field a to distinguishtheir turbulent states betweenactive enrangeof scales,the so-calledequilibriumrange, in which trainment and ultimate dissipation. It is shown that
the energy available from the atmosphereat a given the singularity strength assignedto eachisolatedevent,
scaleis convertedto dissipationin the turbulent break- discernibleabove the reflective background,acts as an
ing wave at the same scale. Whereas a Kolmogorov identifying label, much like frequencyor wavenumberin
cascade model cannot represent the separate centers a Fourier representation. It is argued that the sudden
of dissipationinvolved in a breaking wave field, it is changeobservedin breakingwavesbetweenentrainment
possiblethat an atmosphericcascadeinvolving transfer and runout is associated with a critical state characterstrength.
from larger connectedactiveareasto apparently disjoint izedby a criticalsingularity
A theme running through the fractal conceptualizaimbeddedsubareascarriesboth the spirit of an energy
cascade and the existence of multiscale identities.
As
tion in the sections Fractal Concepts and Analysis is
mentioned above, a spatial representation of the im- that a basic fractal generatorof the Cantor type conage as a Poissonprocesspresupposesa spatial density veys most of the relevant structure of breakingwave
of independent
events. Accordingly,
the Poissonrep- fieldsas we now understandthem. In a companionparesentation, whose average distancebetween eventsis per [Kerman,19934],a modelof an energycascade
is
independent of the scale of representation,that is, the offered to reproduce aspectsof the multifractal strucresolution, is inappropriate to a processwhich is ca- ture of a breakingwavefield basedon sucha generator.
pable of generatingprogressivelysmaller eventsas one
reducesthe scale of inquiry.
Fractal Concepts
All these features of breaking wave field-localized
singularities,self-similarshapes,intermittency, and an
Rather than present a detailed mathematical view
evolutionary cascadeare the hallmarks of a fractal pro- of a multifractal process,we prefer to offer an intuitive
cess.In Kerman and$zeto[1994]it wasarguedthat the viewbasedon a realisticand reusableexample,the Candistribution of breaking waveson the ocean surfaceis
fractal. However, the conceptsand approachusedthere
were for what is known as a monofractalrepresentation
in which one parameter, the fractional dimension",
tor process. Our reasonsare more tutorial; that is, for
geophysicists
who have not been exposedto suchmeth-
ods, than developmental.A reader wishingto study
how suchtechniquesare appliedmay wishto commence
[Mandlebrot,1983],solelyrepresents
the field. This is with the Data section;which describesthe experiment,
16,182
K••AN
AND BERNIER:
MULTIFRACTAL
BREAKING
WAVES
for a discussionof the separationof breaking wavesfrom
the background or with the Analysis section for a discussionof the multifractal properties of the breaking
sentinga (fractional)numberof objectsN and strictly
equatehis iterative scalereductionfactor 1/r with that
here(1/3 eachstep),we haveby his definitionoffractal
waves themselves.
dimension
Monofractal
D
Model
InN
D-
Considerinitially a line segmentof length L, of length
lnr
(3)
[Feder,1988, p. 62]. Superimpose
on L a uniformly which when N - 1/2 and r - 3 are substitutedinto it,
leadsto D - In 2/ln 3 - c•.
distributed weight w whoseintegral over L is
To summarize,a Cantor processhas led to a sequence
of identical amplitude and width singularities,characterized by one value of the singularity strength c• to
whichcorresponds
onefractal dimensionD. Sucha proConsider next a Cantor partition of L whereby the cessis called monofractal. Unfortunately, it is limited
singleinterval is split into three equal length subinterin scopeto describinghow the spaceis redistributedin a
vals of length, I - 1/3. Let us call the originalsegment particular cascade.Next we considera cascadeprocess
the "mother" interval and the subintervals"daughter"
wherea measure,say,local light density,is redistributed
intervals. Consider next a different partition of the in a Cantor-like cascade.
weight w so that the weight of the mother interval is
equally placed on, say, the left- and rightmost daughter
Model
intervals, with no weight on the center daughter. We Multifractal
interpret the assignmentof 0 weight as a death process
Considernext a generalizationof the above Canand withdraw
further consideration of it. We intend
tor process. Let the two surviving daughtersubinterto repeat the process, so let us redefine the partition
o•wdx
-1
(1)
vals,expressed
as a fractionof the motherinterval,be
weightw• - 2-• and the lengthof the daughterinter12,i = 1,2 rather than (1/3) n as above.Similarly,the
val wehavegenerated
as 1• - 3-1.
weight,whichwe preferto call the measurehereafter,
Next considereachsurviving daughterinterval one at
is partitionedto w•, i - 1,2. We againinsiston cona time. Consider the Cantor processapplied to each
servingthe measure,that is,
daughter in turn: first a split to three daughtersof
lengthle - 3- e andthenan assignment
of thesurviving
weightfrom the previousstep,that is, we - 2-e.
When the processis carried to n iterations, the sur-
E w?- 1
(4)
viving intervals1• are of length 3-• with equal weights
It can be shown[Halseyel al., 1986; Feder, 1988,
we - 2-•. We next define the "strength" of each of
p.
85] that after n iterations,thereare C•m segments
these isolated, thin, packed intervals indexed arbitrar(where
C is thecombinatorial
symbol)
of lengthl•• 12
n-•
ily in essence"singularities",by the relationship
n-• , k - 0, 1, ..n. Forexample,
at the
andmeasure
Wl•
W2
(2)
first iteration,n -- 1, thereis onesegmentof lengthl•
and onesegmentof length12. At the seconditeration,
From the Cantor process,wi - 2-n, li - 3-n the sin-
n - 2, thereareonesegment
eachof length1•
2 and1•
wi - l•
gularitystrengtha is In 2/ln 3. FromMandlebrol[1983, andtwosegments
ofl• l•. Thecorresponding
singularity
p. 37], if we considermomentarilythe weightsasrepre- strength after n iterations is found from
Figure 2. Realization
of a fluxcascade
(Besicovitch-Cantor)
fractalgenerator
(w•=0.6, w2=0.4,l• •-0.5,
•2=o.2).
KERMAN
AND
w•w• - (l•l•-•)•
BERNIER:
MULTIFRACTAL
BREAKING
WAVES
16,183
cept is evensimpler: computethe singularitystrength
(5) for
each connected member or "island" defined over its
When (5) is simplifiedby substituting• = k/n, k =
support(spatiallocationof the set), crossreferenceto
0, 1, ..n, which representsan indexing of the total num- like groupswithin an "a-window",and then examine
ber of resulting subsets,
the differentsingularitysubsetsseparately.
Estimation
it can be seen that the singularity strength of the
subset is not necessarilyconstant acrossthe different
su•sets. Similarly, the fractal dimension f of each of
the su•sets formed by different combinationsof I• and
l• and of w• and w• can •e expected to vary with
We do not carry the analysisto the calculationof •(•)
of Fractal Spectrum
The singularitystrengtha of (7) is a measureof how
much one has to stretch the spacein the vicinity of a
non-differentiable function to achieve bounded behav-
ior. The largerthe singularity,the smallera is, and
the greateris the necessary
stretching.Accordingly,
in
and f(•) or equivalentlyf(•(•)).
What we wish to indexingvariousintervalsin the previoussection,the
stressis that a generalizediterative procedureh• led singularities
can be reconsidered
in orderof their sinto imbeddedsubsetsof different fractal properties. Such gularbehavior;that is, monotonically
with increasing
a processis called multifractal.
An example of such a c•cade is given in Figure
Distinctive features of the graph include the isolated
peaks and their intermittency. Not so obviousmay •e
the existenceof commonamplitudesand widths to
sets of singularities. These geometric features and the
fact that they stem from a c•cade processare common
to the qualitative •pects of breakingwaves• discussed
in the Introduction.
An equivalentprocessis to stretchthe function,not
its support,by raisingthe functionprogressively
to a
givenexponent
q,referredto astheqthmoment.(Considerq to be positiveinitially in accordance
with our
implicit assumptiona < i whendiscussing
stretching
asopposed
to contraction.)As thefunctionis stretched
vertically,the singularityfor the ith supportinginterval
originallydescribed
by o•i(q-- 1) is nowdescribed
by
ai(q), where
Fractal Singularity Filtering
o•i(q)• ai(1),
(q • 1)
(S)
Forthe verticalstretching,considera uniformchange
The conceptof fractal singularity filtering follows directly from the conceptof imbedded subsets. Consider ofscale
I•(q)ateach
ofthennontrivial
intervals
where
a positive-definite measure/• supported on an interval v is uniquelyselected
to conserve
the originalmeasure,
of length i at N nontrivial subintervals. We first nor- that is,
malize the measureso that its integral over the domain
•..•Yi'i -- 1
(9)
is unity and then compute an integral of the measure
E•li --• q'•'(q)
overeachisland,say,/•i, and relateit to the island(interval) lengthli by the relationship
i=1
i=1
For an analytical process, such as the Cantor pro-
cess,where /•i and li are known and countable,v(q)
The definitionof singularitystrengthin (7) can be
better understood in terms of local density, say, the
amountof light emanatingfrom a remotesensor'sfoot-
can be found by solution of a transcendentalrelationship, called the partition function.
It remains
to relate
• to the fractal
dimension
and
singularity strength of the various subsets. Consider
by
printor pixel,represented
as,say,yii•-1. Forareasof [Feder,1988]somefractalsubsets$a characterized
constantdensity,ai -• 1. However,for local peaksof a and their union
S = t3,•S,•
(10)
density,if the apparentdiscontinuityis largeenoughin
the limit, it is necessaryfor any li to have ai --• O. In
Consider the measure relabeled to a number of sets
other words, the senseof the singularitystrength a is N(a) for a betweena and a 4-5a. At someinterval
inverseto the commonnotion of density: the larger the length 5 (• all li) usedto coverthe sets,one expectsa
(discontinuityin) local density,the smallerthe singu- relationship
larity strength.
In the above Cantor example there would be numer-
ous,in fact, C• (wheren >> 1) subintervals,
each
with a common value of a. We then consider all those
N(o•,5) - N(o•)5
-.t(•)
(11)
wheref(a) is the fractaldimension
of the subset.Con-
memberswith a singularitystrengthsa betweena and sider a redefinition of a based on the available resolution
a + 5a and relabel them • the a subset. Such a pro- in the form
cedure is equivalent to Fourier filtering in which we
/•i = 5•
(12)
identify one frequencyor wavenumberband of interBecausethe set elementsare countedonly at locaest, excludeall others, and examinea narrow band representation of the function by sliding our filter along tions
where/•i
• 0,necessarily
•NmN(a,5)[.]- •[.]
the frequencyaxis. The fractal singularityfilter con- Nm is the maximumnumberof setsat a givenresolu-
16,184
KERMAN
AND BERNIER: MULTIFRACTAL
BREAKING WAVES
tion). Thereforeupon substituting(12)into (9) rewrit-
of the Canada
ten for countability, we have
nine sorties over the Atlantic and Bay of Fundy. The
Centre
for Inland
Waters
was flown on
linescancameraestimatedthe light in a pixel footprint
N,•
E N(a)5•q-•(•)+•'(q)
=1
somewhat less than 0.8m 2 over a swath of about 570
(13) m along a path about 30 km long. The best contrast
between the breaking waves and the background was
This sum, now over all subsets,receivesmany of its found at 0.95/•m. The treatment of the imagery and
contributionsfrom terms belongingto a specialsubset more details of the experiment are given by Kerman
in which5'•q-I+•' isa maximumfora givenqor in which and $zelo, [1994]. An exampleof the imagerytaken
over the Bay of Fundy is given in Figure la for an area
0
o•qa-f(a)+r(a(q)))•-•- 0
about 400 m on a side.
(14)Background
In (14), a,• succinctlydefinesthat specialsubset
in which the maximumoccurs. To have (13) remain
Process
To examine the fractal propertiesof the image, we
boundedrequiresthat •qa.•-](a.•)+r(q)remainfinite must first eliminate thoseaspectswhich are nonfractal.
The method usedin this sectionto accomplishthis separation utilizes the optical scatteringspectrumof images
and nontrivial as 5 -• 0, which requires
r(q) = f(a,•) - qa,•
(15)
at different thresholds and the statistics of the weak but
spatially extensivebackgroundprocess.
The meaningof r(q) followsfrom (9) and (12), in
The first problem in the identification sequenceis how
whichwe note that N(q, 5) is givenby
to separate areas of clearly different reflective properties; that is, specularreflectionarisingfrom tilted waves
and scatteringfrom bubble-infestedpatches. As menN(q,5)- •• - 5-•(q)
(16) tioned
above, we have utilized two propertiesof the imi=1
ages' their optical spectra and their cumulative stathat is, the number of boxes required to cover the qth
tistical structures. In the first case, various images
momentof the me•ure y at spacing
5 varies• 5•(q).
[Kermanand $zelo, 1994]of the samesceneat each
We therefore•sociate v(q) with the (covering)dimen- of seven optical wavelengths,were analyzed at differsion of the qth moment of the measure and derive it
in the customary box-countingmethod of fractal anal-
ent percentliesof the cumulative probability functions
(cpf) corresponding
to differentareal extent or coverysis. We emph•ize that N(q, 5) relatesto the covering
ageof the total scene,rangingfrom 25 to 0.05%. The
of a measure and not its support, which is restricted to
intensityof eachwavelengthfor a giventhresholdcorreq = 0. It alternatively is the moment of the measureof
spondingto a given areal extent is presentedin Figure
order q evaluated at resolution 5.
3 as a function of optical wavelength.
From (14) and (15),
For each threshold the intensity decreaseswith optical wavelength. However, the rate of decreaseis less
a• =
Or(q)
Oq
(17)
whichprovidesa methodto extract am givenv(q) by
meansof (16). The fractal dimensionf(am) is then
calculatedfrom (15).
It is convenient
to consider
an extension
of the above
>.5.0•
method to the coveringof are• rather than a line •
discussedabove. By redefining 5 to be an incremental
• ,3.0
area and reconsidering
a(q) and v(q)in (12) and (16),
•
2.0-
0
1.0-
-r
_
the b•ic result is preserved. Such a structure which is
more natural in definingthe singularity propertiesof a
spatial area, also allows us to considera set of points
distributed over an area in the same way one considers
a Cantor set distributed on a line. The similarity also
allows below for the construction of a c•cade
model in
i-
z
4.0
Coverage from
•,25
25% to 0.0488 %
(byfactor
of2)
a singledimension,whichis actually area.
channels
I to 6
run 7
Data
I
o.5
Experiment
0.6
i
0.7
I
i
o.8
o.9
1.0
WAVE
LENGTH
(lam)
The imagery to be utilized in this study was gath- Figure 3. Intensity of image at different optical waveered in March 1984 over the ocean near Nova Scotia, lengths. The image has beenthresholdedto achievedifferent
Canada. A linescanner mounted on the DC-3 aircraft
areal extent and averagedlogarithmically.
KERMAN AND BERNIER:MULTIFRACTAL BREAKINGWAVES
with increasingoptical wavelength,at least aboveabout
0.67 #m, and with increasing threshold. Clearly, as
the image becomes brighter, it also demonstrates an
increasedsensitivity at larger optical wavelengths.
If the processwas entirely reflective, one would expect the spectra to continue to mirror the product of
16,185
its cumulativeprobability function (cpf). An example
of the cpf from flight 7 is providedin Figure 4. As
discussed
in Kerman and Szeto,[1994],the well-defined
linearsubrange
of the cpf,herebetweenabout0.1 (10%)
and 0.005 (0.5%), can be shownto be statisticallyinvariant to averagingat different length scalesand has
the imposedlightingspectrum(directsolarand skyra- been identified as fractal.
The question arises as to what, if any, structure the
diance)and the surfacereflectioncoefficient.In sucha
scenario,as the image'saveragebrightnessis increased, weaker intensity region possesses.When the cpf of an
entire image is replotted linearly against intensity I on
subelements
maintaintheir similarity(hereparallelism) a standard "probability graph", that is, as a test for a
with the weakest(herethe mostextensive)image. Such Gaussianstructure, the curvesare invariably straight
is not the case. We conclude that there is an additional
up to 70 to 85% accumulation,suggestingthat some
distribution(i.e., positiveintensityonly)
sourceof light exiting the breakingwavepreferentially quasi-normal
might be present. On the other hand, if the cpf is replotwith increasingwavelength.
The uppermostfour or five curves,ranging in extent ted linearly againstIn I, the resultinglocusis againlinfrom 0.05 to about 0.78% are virtually parallel. In other ear, suggestingthat a log-normaldistribution might be
words,as the image elementschosenare brighter in the applicable. However,neither distributionis meaningful
senseof total light overall wavelengths,the effectivere- for the process. The Gaussian distribution, conceived
flectances of different size elements remain unchanged of as many additive subeffectscombinedin a singleobat eachwavelength.Also the fact that the optical spec- servable effect, implies no limitation either positive or
tra at the longestwavelengthsessentiallymaintain their negative to the observedvariable, whereasintensity is
parallelismleads us to suspectthat even at such large clearly positive definite. The log-normal process,concoverageas 25%, the imageat longwavelengthsis dom- ceived of as many multiplicative subeffects,is usually
applied only in the large variablerange. We believeit is
inated by a nonreflective process.
We ascribe the apparent source of light at longer not justified in the lower-intensity process,which more
wavelengths
to the scatteringprocessof bubbles[Davis, likely arises from an additive rather than a multiplica1955]both underand abovethe watersurface.We here- tive effect. Also, even though a log-normaldistribution
after refer interchangeablyto the reflective processas appearsto be a good qualitative fit to the cpf in another
the background processand the scattering processas subrangeat muchlarger values,say,for the largest 10%
the bubble process.
or so,we preferto ignoreits relativelygoodperformance
The second element of the method to discriminate
at larger intensitiesin favor of a fractal representation.
betweenthe reflective and scatteringprocessesinvolves
We hypothesizefor the weak-intensityregion a ranthe curvesof the rarer but presumably more reflective
-1
w
-2
-5
-6
0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1.6
1.8
2.0
LOG10 INTENSITY
Figure 4. Cumulative
probability
function
forpixelintensity
(wavelength,
0.95/zm)forflight7.
16,186
K••AN
2.5
AND BERNIER:
I
I
MULTIFRACTAL
I
I
I
BREAKING
I
I
WAVES
I
I
2.0
1.5
--
--
--
• 1.o
n-
OBSERVED
CUMULATIVE
•..•
FUNCTION •
PROBABILITY
n- 0.5
-
•
--
z
OI
•©•
BESTFIT
-1.0
1
2
3
4
5
6
7
8
9
10
INTENSITY
Figure 5. Inverse Rayleigh function transformationof cumulativeprobability function versuspixel
intensity. Deviationfrom a linear relationshipat weakestintensityinvolves< < 0.1% of area of the image
and resultsfrom digital round-offand dropouts.
domreflectiveprocess
whosevectorphasorhasrandom,
Gaussian-distributed
amplitudesandrandom,uniformly
distributedphases. We associatethe Gaussianaspect
of the descriptionwith the nearly Gaussiandistribution of waveheights[Longuet-Higgins,
1983]in sucha
mannerthat the smallestimagepixel hasmany additive
The questionarisesasto wherethe relationship
fails.
We havearbitrarilydefinedan equivalentsignalto noise
ratio for the method by consideringthe ratio of the
actual cpf to the best fit Rayleighdistributionbased
on the weightedlowest90% intensities.When the ratio reachesa prescribedvalue(usually2), we selectthe
subresolution sources of reflection associated with tilted
nearesttabulated intensity correspondingto the nearest
facets. The uniformly distributed phasesare thought
to arisefrom the original wavefacetswhich are both
weakly correlatedspatially and of indeterminateand
nonpreferentialphase.
The resultingprobabilitydensitydistributionof am-
20
18-
plitude
follows
aRayleigh
distribution
given
by
pdf(I)
=I ezp()
16-
(lS)
• 12-
whose
cumulative
function
cpf(I.),is
cpf(I)
- 1- ezp(--•-)(19)
12
and whose inverse function is
4-
I -- {-2/n(1- cpf(I)}1/2
(20)
2-
Accordingly,
if any cpfis indeedRayleighin formand
0
I
I
I
i
i
the functionalform on the right hand side of (20) is
-6
-5
-4
-3
-2
-1
0
plotted againstI, a linear relationshipis expected.An
LOG1oCUMULuLATIVE
exampleof such a graph of the lower-intensityregion
of an imagefromflight 7 [Kermanand$zeto,1994]is Figure 6. Ratio of measuredcumulativeprobabilityto inpresentedin Figure5. Indeed,the relationshipis linear verseRayleighfunctionbasedon structurein 90% of image
in all casesfor at least 90% of the image.
areaand plottedagainstaccumulated
area(coverage).
KERMAN AND BERNIER: MULTIFRACTAL
1(•ø
16,187
The enhanced lighting is visualized as arising from
the multiple scattering of photons within the bubble
cloud on the breaking wave'sface. For a given illumination, the deeper the cloud and the more concentratedits
bubbles,the more scatteringis possibleand the brighter
the wave appears. Accordingly,the sampledlight level
representsa natural vertical integral of reflectanceover
>- lff 1_
<• 1(•20
the bubble
Cumulative
4_
cloud above the local
function
Run 7261
ld 5_
rate of turbulence
I
I
I
I
I
10.-2
Illl
"undisturbed"
water
level. As shown later, the depth, the horizontal dimensions, and the bubble density vary systematically
throughout the lifetime of a breaking wave. It is to be
expected that the scattered light also varies during the
wave'slifetime and momentarily reflects the production
probability
•
BREAKING WAVES
I
I
I
ld I
I
I
Illl
I
ld ø
and bubbles.
We begin our analysis of light intensity and scale
by consideringthe accumulationof light and the area
of the islands(patches)left after the thresholdoperation against the background. Each island was formed
by
joining all neighboring(eight-connectedness)
pixels
Figure 7. Cumulative probability function showingbest
INTENSITY
fit Rayleighregion(opencircles)and fxactalregion(closed with intensity above the threshold. Each island's accumulated light and area are computedin terms of the
circles).
respectivesum over the total ensembleof islands. The
fractional light and area of an individual islandare then
coverage
and useit as a thresholdof the imageagainst comparableto the measureover unit interval as discussedin the Fractal Conceptssection. We denote as Ii
the backgroundRayleigh process.
The procedure is demonstratedin Figure 6. For the fractional light arisingfrom the fractional area Ai of
about 90% of the imagefrom an areal extent of I to 0.1, the ith island. The correspondingsingularitystrength
the ratio of cpf valuesis unity and then risesrapidly. ai is then defined by
We selectthe arealextent(coverage)nearestto the ratio of 2 and find the associatedthreshold from the cpf.
The same result is displayedin Figure 7 for the cpf
itself. The changefrom weak reflectivebackgroundto
stronger,scattered,fractal processoccursat the boundary of the two charactersets. In hindsight a weak inflection point in the cpf may be noted which was not
obvious a priori.
We conclude that
a self-consistent
method
exists to
Ii - A•'
(21)
The c•i valuesrange from about 0.85 to 1.05 for the
variousflights of the experiment[Kerman and Szelo,
1994].The probabilitydensityof c•is presented
in Figure 8 for severalof the flights. Clearly, there are many
more larger c• eventsthan smaller ones. The question
as to the physical differencebetween different c• islands
naturally arises.
extract the fractal (scattering)processfrom the background(reflective)process. Our method is basedon
first identifying in the optical spectrum two inherently
different(reflectiveandscattering)propertiesof the surface. Second,the method relies on a sharp changein
To examinethat question,considera reorderingof the
c•i from smallestto largest. Figure9 demonstrates
how
the light and area are accumulatedprogressively
from
c•minto C•ma•.The two curvesshowcomparablebehavior' risinglessrapidly initially overthe sparsec•islands
the detailed inverseof the cpf structure comparedto an and then accumulatingrapidly overthe densesets. The
extensiveRayleigh distribution to identify the lowest light accumulationexceedsthat of area, gainingmost
intensitiesof the fractal processwhich are statistically of its advantage
for severallargebut abnormallybright
identifiableagainst the background.
events. The advantageis progressively
overcomeas the
large a events are considered. The difference between
Analysis
Fractal Singularities
The most characteristic feature of a breaking wave
field is the pattern of bright patches against an otherwise dark background. While there is evidence of
shading within the background,very possibly associated with bubble cloudsconsistingof sufficientlysmall
bubbles with terminal velocities comparable to or less
than the turbulent velocities left in the breaker's wake,
it is the isolated patches which offer good definition
comparedto the reflective process.
the fractionalaccumulatedlight and the areais alsodisplayedin Figure9. If the light originatingfrom a patch
was always proportional to its area, the curve would
be identically 0. Initially, with eachnew area at small
a, the light accumulatesfaster until it reachesa maximum disparity. Thereafter light accumulatesslower
than area. The questionnow is, what is the difference
betweenc• subsetsto the left of the maximum, which
contributemorelight than area,and thoseto the right,
which have the oppositetendency?
It is usefulto considersomelaboratoryexperiments
on the growth and decayof breakingwavesto try to
establishwhat interpretationto give to theseresults
16,188
KERMAN
AND
BERNIER:
MULTIFRACTAL
BREAKING
WAVES
0.3
c
0.1
o
i
0.9
0.95
I
1
Singularity Strength
Figure 8. Probability densityof c•subsets.
(Figure 9). Replottedin Figure 10a are somedata of This normalization leads to the maximum area occurPapanicolaou
and Raichlen[1988]for the growthof the ring at aboutwt - 0.75;that is, at an agefor about0.75
sideview area of a surf breaking wave for various tank of the prebreakingwaveperiod. It alsoimpliesthat the
configurationsrangingfrom a beachslopeof 0.6 to 2% effectivephasespeedof the breakingwaveis about 0.8c,
and an initial wave height to a water depth ratio be- in which c is the prebreakingphasespeedin accordance
tween and 0.4. In their analysis those authors demon- with the measurementsreported by Melville and Rapp
strate a similarity in the size of the bubble cloud with [1988](Figure 10). Melvillealsoreportsa well-defined
structurein the scalingbehaviorfor the initial entraintime after initial breaking.
The geometric similarity apparent in the original ment ending near wt = 1. Thereafter the turbulence
plots has been extended to nonshoalingwavesby not- is found to slowly relax to the intermediate asymptotic
momentumless
wake[Tening the critical relationshipin suchshoalingexperiments regimefor a two-dimensional
between depth of initiation hb and the wave'samplitude nekesand Lurnley,1972,p. 124].
Hb'
Hb--0.8hb
Kerrnan[1988;1993b]haspresented
datawhichclearly
(22)show
that the maximum of the integrated sound field
[Galvin,1972]basedon numerousexperiments,
and the under a breakingwave occursat a time after initiation
relationshipinvolving the wavelengthat breakingAb
Hb_ 0 14tanh hb
- '
about 0.4 of the waveperiod. It is thought that the rate
of bubble entrainment
and hence the rate of increase of
the bubble cloud size are directly proportional to the
soundlevel and that suchproductionwill thereforepre-
for shoalingwaves. After a transformationof variables cede the observed time of maximum bubble cloud size.
It was also noted that the sound radiation
into the air
comparedto that into the water noticeablybeginsto
increaselocally at about wt = 1. This result is ascribed
the solution of the transcendental equation is approxi- to the presenceof bursting bubbleson the surfacein
mately y - 0.5, or the aspectratio hb/Abis about0.082. the runout stagewhich radiated only into the air.
y- 2•rA•
KERMAN
AND
BERNIER:
MULTIFRACTAL
BREAKING
WAVES
16,189
-0.12
-0.1
0,7-0.08
0.6-
o
o
-0.06
0.5-
o
o
0.4-
o
-0.04
0.3-
0.2-
-0.02
0.1-
alpha_crit
0.8
0.85
0.9
0.95
1
1.05
1.1
1.15
1.2
Singularity Strength
Figure 9. Accumulationof light and area and their differencewith collectionof subsetsfrom c•mi,•to
From these various experimentswe concludethe following.
1. The changeof scalingand of the differencein the
acousticgenerationin air and water are clear evidence
of an entraining and a dissipating(wake) stage within
a breaking wave. The end of the entrainment stage
occurs near cot - 1, with evidence of the asymptotic
decaystage after cot- 5.
2. The maximum bubble cloud area viewed laterally
occursat a time cot= 0.75 which, within the potential
errors associated with systematic differences between
the experiments, is essentially the time of the entraining/dissipatingcrossover.
to broken-uppuddlesof foam at larger a. Conceptually, for entrainmentwherethe densityand thicknessof
bubblesis above averagefor the whitecap transient as
a whole,the light densityis aboveaverageand the sin-
gularitystrengthis belowaverage.Conversely,
in the
dissipativerunout, asfoamholesbeginto appearwhen
the wave becomesspatially thinner, the light densityis
reducedand the singularitystrengthis increased.At
the critical crossoverpoint, for ac - i the fractional
light is directly proportionalto its apparenthorizontal area,indicatingthat the processes
determininglight
and area are balanced, as also seen in Figure 9 previously. Hencethe critical value of a is a consequence
of
the balance between entrainment and dissipation.
We therefore associate the maximum
difference in
Such a division is the basis of the conceptual differlight accumulationover area accumulationdiscussedin
ences
betweenwhitecapsand foam as expressedin the
conjunctionwith Figure 9, with the critical stagewhen
literature.
The importanceof the developmenthere is
the breaking wave has built up its maximum volume
that
the
distinction
can now be expressedquantitatively
of bubbles,which impliesa maximumin the light scattered. Thereafter the area continues to increase, but in terms of reflectance contributions over the area conthe volume and the amount of light scattereddecrease. tributions of connected fractal subsets. The individualThis criticalentraining/dissipating
crossover
is unique- ized identificationof the stageof developmentof each
ly referencedby the value at the maximum light and breakingwaveallowsfor individualextractionand maarea disparity, which is defined as c•c. From Figure 9 nipulation of wavesof comparableages,albeit of difthe maximum occurs at ac • 1. Further, for a < ac, all ferent sizesdependingon the initial energyavailableat
a subsetsare primarily entraining, and for a > ac, all their creation. We refer hereafter to such a processas
subsetsare dissipatingmore than entraining. The sin- singularityor a-filtering.
The processis outlined in Figures l a to l d for flight
gularity strength is a monotonicfunction of the breaking wave'sage, from fresh youngbreakerswith small c• 7 [Kerrnanand Szeto,1994]. The first transformation
16,190
K•••
AND BERNIER: MULTIFRACTAL
BRE•NG
WAVES
INCIPIENT
2O
BREAKING
P1
•
10-
,.
X/hb=O.O
••191
0
P1
hb= 13.50cm
Hb=16.50cm
X/hb= 2.0
FRAME
43
-10 i
-60-50-40-30
'-20-10
0
10
2o
3o
4o
-20-10
i
i
0
10
I
x (cm)
ENTRAINMENT
2ø1
!
10-1
•
0
10
I
BUBBLE
•
e•,•'"PLUME
[•:¾•:'.:.:::.%.
20
.,,,,
..........
I
30
20
/
P1
x/h•,=4.0
10
I
40
r..
201
1F1
-J
E '" [
i
60
I
i
I
I
I
50
60
70
80
90
1co
50
P1
xlhb=7.0
I
60
I
70
I
80
I
90
I
I
I
I
I
100
110
120
130
140
X (cm)
DISSIPATION DOMINATED
X/hb
P=120'0
I
x/ hb=10.0
•:'?..'•._...?•?'•'(':•i•!i!!•':.'%'"•,.-.
_,, FRAME
234
"•••'""•'
....
-'••••
'"'•..•
'.'.
N
0
lO-•
...;..., ..•.•.., ......
, , , , , ,•, ,
•0
8O
'
FRAME
172
P1
•00
70
-10
-.,,,,--.
i
.,........:•::.:•
0
90
i
50
..,,•..
..:.':'•
•:.;•,:,.%•.•
I
20-
o •"-•
•
•
1
X (cm)
•
i
40
x (cm)
"•'L,..• FRAME
92
........
I
I
30
DOMINATED
•
-10
i
20
•20
•30
•40
•50
•0
•70
•80
x (cm)
,•'.•:.:•..':•:..;••
•.• -•.....:•
FRAME483 1
I
-10 210
2•0 2•0 2•0 250
' 260
' 270
' 280
' 2•0 300•
'
310
x (cm)
Figure 10. Growth of sideviewarea of breakingwavein laboratory tank with scaledage after breaking
(wavephase). From Pavanicolaouand Raichlen(1988).
of the image (Figure lb), consistsof a thresholdto
removethe reflectiveRayleigh backgroundand is presentedwithout regard to its singularitystructure. The
probability distribution of number, area, and brightnessof all alpha categoriesis presentedin Figure 11.
As noted with Figure 8, the numberof large a islands
greatly exceedsthe number of small a islands. The distributions of area and brightnessbetweenthe minimum
of about 0.85 and the maximum of 1.05 are essentially
tensive whitecap coverageexperimentssummarizedby
Monahah and O'Muirchear'laigh
[1980]. In Monahah
[1993,Figure la, equations(1) and (2)] the measured
partition betweenactive breaking wavesand the total
whitecap coverageis about 0.14 comparedto the estimate here of 0.2. The best estimate
based on a collec-
tion of numerous experiments is that the active white-
capswill occupyabout 0.85% of the area comparedto
the aboveestimateand 0.68% of the area whena _• ac.
identical and indicate a consistent functional structure
The agreementbetweenthe techniquesis remarkably
at least for a _• a•. However,they displaya crossover good consideringthe independenceof the methods. The
near a - a• - 1 that is associatedwith the arguments commontechniqueof making whitecap coverageestiof the entrainment/dissipationbalanceabove. Clearly, mates is to establisha thresholdfor a given image at
the dominantcontributionto the arealextent and light an intensity related to, at best, a critical reflectivity.
scattered by actively breaking wavesis from the more This procedure is essentiallywhat has been achieved
in our study, albeit from a differentperspectiveinvolvmature events near etc.
The connectedsubsetsfor a • 1 are presentedin ing the statisticalstructureof the backgroundand inFigure lc. The entraining breakingwavesfor the con- tense regions. Where the difference occurs is in the
dition a ( 1 are presentedin Figure ld. The brightness treatment of the individual patches where our discrimcontribution and areal extent of total fractal coverage inator utilizes a nonlinear parameter, the singularity
are 8.7 and 3.4% and 2.0 and 0.68%, respectively,for strength, basedon integral propertiesof the patch; that
the entraining, whitecap subsetsalone. The estimates is, its total light and spatial support. Our estimate
for total areal coverageare consistentwith other esti- of the whitecap/foam ratio is most critical to the esmates (6.3%) for the samewind speed,basedon ex- timate of the threshold of fractal activity comparedto
KERMAN
AND BERNIER:
MULTIFRACTAL
BREAKING
WAVES
16,191
0.3
0.1
i
I
0.95
1
SingularityStrength
Number
• Area• Light
Figure 11. Probabilitydensityfunctionof number(solidtriangle),area(solidbox) andintensity(open
box) of connectedsubsetsfor givena categories.
the Rayleighbackground.It wouldbe usefulto arrive algorithm to select the best fit partition parameters
at an estimate of the threshold in terms of local con-
finds the case of minimum
nectivity rather than imposinga global threshold. We
neverthelessconcludethat the singularityfiltering procedureallowsfor a systematicevaluationof individual
breaking-waveeventsin terms of their turbulentstate
with an accuracycomparableto that of existingmeth-
the calculatedf(a) and a and their exact valuesfor a
givenorderof (positive)moment.The error in fitting
the fractal spectrumto • Besicovitch-Cantorprocessis
typically small (0.019-4-0.007).
ods.
Fractal Spectrum
accumulated
error between
The results of a secondtest to evaluate the accuracy
of the recoveredli and wi are also presentedin Table
1. The estimated I and w are comparedto the exact
solution. Again the averageerror is small, typically 4
to 8%. Accordingly,it was concludedthat the comBefore estimating and analyzingthe fractal proper- puter codewas accurateto better than 10% and that
ties of the image data [Kerrnanand Szeto, 1994], a any structurefoundby subsequentprocessingof the imcalibration of the computer code to calculate the frac- age data to vary by more than that amount was likely
tal dimensions of subsets with a known result was arto be dominated by the processand not the numerical
ranged. An analytical expressionfor the fractal spec- analysis.
trum of a cascaded
flux (Besicovitch-Cantor
(BC)) proThe best test of a multifractal processis probably
cess,describedin the Multifractal Model section, has whether the successive
momentshave the scalingstrucbeenfoundby Halseyet al. [1986]. It thereforere- ture aspredictedby (16). Severalexamplesof the summained to generaterandom realizationsof the BC pro- mations over different moments from -2 to +4 for differcesswith knownpartitionproperties(li, wi, i = 1, 2), to ent boxsizesfor a givenflight (7) arepresentedin Figure
calculateits fractal spectrum, and to solvefor its I and 12. The log-logplot of N(q, •) is quite linear for small
w parameters.
positive q for a range of box size from about I to 512
Table I presentsthe resultsof an error study for fixed pixels(400 m). As the order of the momentincreases
li andwi for 128sections
of 6562(3s) pointseach.The positively, a perturbation occursnear a scaleof about
16,192
KER]V[AN AND BERNIER: MULTIFRACTAL
Table
1. Results of Fractal Parameter
Estimated
Mean
Variable
Multfractal Spectrum
Extraction
Estimated
Standard
Deviation
_
Exact
0.019
0.007
Wl
w2
0.629
0.374
0.068
0.068
0.600
il
12
0.482
0.225
0.150
0.112
0.500
Estimation
BREAKING WAVES
Error
0-
0.400
-1-
0.200
4-2-
Error analysis of estimated spectral spectrum and
Besicovitch-Cantor parameters based on 128 independent
realizationsof length3s.
-6-
32 m and increasesin amplitude as q increases. This
-7
deviation is believedto arise from a periodicity in the
-•' • ' •
4 (• • 10 12
-4
data imposedby swell,with a wavelengthof about 65 m
ORDER OF MOMENT
modulatingthe localizationof the breakingwaves.The
analysis for negative q is less convincing. The source Figure 13. The coveringdimensionr(q) of the various
'
of error in this case is believed
to be the truncation
of
order unity integersof the sampleddata so that there is
almost no dynamicrange in the successively
compacted
data implied by negativeq.
The scaling exponentsof the coveringsfor different
momentswere then computedfrom the best log-logfit
to each moment and are plotted in Figure 13 for the
total range of q used, as discussedbelow. Becausethe
accumulationwasoveran area and not an intervalalong
a line as implied in (16), the box length was replaced
with box area for consistencybetweenimbeddingdimensions.
To safeguard against meaningless,nonphysicalderived parameters, the subsequentderivation of c• and
f(c•) wasconstrainedto acceptonly that rangeof q for
which
(1) a(q+6q)<a(q)(2) f>0(3) 0•_<0.
These ]imitations were alsoimposedby Meneveauand
I
'
'
'
I
'
moments associatedwith summationsas in Figure 12.
tifractal spectrumderivedfrom r(q) by the methoddescribedby (15) and (17) is presentedin Figure 14 for
the acceptablerangeof q (4 •_ q •_ -2). The spectrum's
main feature is its maximum(f = 0.8), whichoccurs
near c• - 0.9. The fact that the spectral maximum is
less than unity results from the thresholdingprocess,
whichin essencenullifiesthe existenceof the (breaking
wave-foaming)processin distinct regionsof the image.
Qualitatively this result agreeswith our intuitive notion
that the breaking of waves is sparse, that is that the
breaking occurs "almost nowhere". In a similar analysis for the dissipationwithin Kolmogorovturbulence,
Meneveau
and Sreenivisan
old for their
data
did not establish
and arrived
a thresh-
at the conclusion
that
Sreenivisan[1987a]in their analysisof time sequences their estimate of dissipationwas spacefilling. For us to
of estimated turbulent dissipation. The resultingmul0.8
2O
q4
z
Z
o
3
15-
G
0.6-
z
•
1o-
z
5-
o
•
o-
2
:•
_
• O.4n-
• o.2-
o
I
I
2.00
I
I
4.00
I
I
6.00
I
I
8.00
LOG2 BOX LENGTH
Figure
from-2
-
i
o
I
10.00
i
0.4
i
0.6
i
i
0.8
I
i
1.0
i
i
1.2
i
i
1.4
i
1.6
ALPHA
12. Summations associatedwith order of moments Figure 14. The fractal dimensionf(c•) of the supportof
to 4 at different box sizes.
different subsetsof singularity strength c•.
KERMAN AND BERNIER: MULTIFRACTAL
hypothesizealternatively that breaking occurs almost
everywhereand that we are incapableof sensingthe
many smallerand weakerbreakingwaves,includingthe
so-calledmicrobreakers,ignoresthe resultsof the Data
section that there are two distinct intensity regions,
both physicallybased. We also note that in Figure 14,
BREAKING WAVES
16,193
like generator. This aspect is not required in the bino-
mial multiplicativeprocess[MeneveauandSreenivisan,
1987b]usedto representturbulence.Further, because
the processis multifractal we require a method to generate a distributionof subsetswith differentsingularity
strengths after many iterations. Accordingly,we need
a(q = 0) corresponding
to fma• is lessthan unity in- to considera generalizedfractional split of the origidicatingthat the dissipationconnectedwith turbulence nal motherinterval(seethe Multifractal Modelsection)
in the breaking wavesis distributed over noncontinu- and the assignmentof a fractional transferof the meaousspace(fractalsubsets)and that thereis no concern sure from one generation to the next. This brings us to
about the finitenessof the energeticsas discussedby the lowestorder of complexityfor the fractal generator
Meneveau and Sreenivisan.
which will have a multifractal spectrum.
Because the fractal spectrum of such a process is
Several other significant dimensionsare included in
Figure 14. The correlationdimensionfor q - 2 is 0.67, known analytically we can attempt to fit the observed
while the informationdimension(q - 1) is 0.74. The spectrum as describedin the Fractal Spectrum section.
former dimensionis important in describingnearest- It turns out that the fitting processis realistic and acneighbor distancesand pairing, while the latter leads curate, particularly if one ignoresthat part of the specto an estimateof the informationalentropyS [Feder, trum for q where the data quality makes the derivation dubious. In arriving at the parametersof the BC
1988,p. 78] givenby the relationship
process, it is useful to reconsider an interval as an area
which is being partitioned and the assignmentof weight
to a daughterinterval (area) as a fractionof a flux exof S = 4.6. (f• = f(q = 1)). Also as demonstrated isting at the mother level. We hereafter redefine wi and
by Feder, most of the subsetstend to concentratenear li of the Multifractal Model section as Fi and Ai to
c• = 0.74 for q = 1. The subset density in this re- represent fractional flux and area. The nature of a BC
gion may be related to the estimated critical singular- processallows for 2 subprocesses.Without recourseto
ity strength for crossoverfrom active entrainment to a physical model, the significanceof thesesubprocesses
runout as describedin the Fractal Singularitiessection.
is unknown. We simply refer to them as subprocesses
Another distinct feature of the fractal spectrum is
I and 2 and arrange them so that subprocess1 is that
the rapidly decreasingfractal dimensionof the support processfor which most of the flux is carried. As such it
of subsetswith c•(q) < c•(0). A minimumsingularity might be called the flux-dominant subprocess.
strength of about 0.59 is predicted from the projection
Table 2 summarizes the results of a best fit of the BC
of Figure 14 to f = 0. (The projected maximum of processto four flights of the aircraft at a range of wind
about 1.6 is believed to be subject to experimental limspeeds. Flight 12 was taken relatively closer to shore
itations and thereforepoorly resolved.)If one accepts than the other flights, and its statistics may relate to
the hypothesisthat the evolution of a breaking wave
an effectivewind speedlessthan the 19 m/s listed. The
is describedby /••- c•,•i, [Kerman,1993b],the overall trend is that the flux and area partition of subincreasingfractal dimensionwith Ac• may also be as- process1 increasewith wind speed,while the partition
sociatedwith the increasedprobability of samplinga parameters of subprocess2 compensateand decreaseas
breakingwave(i.e., they covermore space)as the rate the wind speed increases. In other words, as the wind
of evolution of the breaking processdecreases.
speed increases the flux balance shifts in favor of the
flux-dominant path and its larger areal fraction.
Flux Cascade
Model
A cascademodelbasedon Phillips's[1985]concepts
of input, dissipation,and energyflux by wave-waveinIt is instructive to enquire whether a simple model teractionshas beenpresentedby Kerman [1993a]. In
suchasthat stemmingfrom the pioneerwork of Besicov- his developmentof an equilibrium subrange in waves
itch and Cantor[Feder,1988]mightbe applied.Clearly with length scalesdistinctly smaller than those of the
the processwhich we wish to mimic exists at distinct most-energeticwaves and larger than those for which
locations and is 'dead' over most of the area, necessi- the drift current exceedstheir phase velocity, Phillips
tating the inclusionof a trivial interval in a Cantor- considersa local balance in wavenumberspacebetween
$ = -flUff1
Table
Flight
2. Flux and Area Cascade Parameters
Wind
Speed,
m/s
05
06
07
12
12
17
17
19
F1
0.621
0.854
0. 786
0.771
Cascade
1
A1
fl•
0.738
0.904
0.859
0.848
1.56
1.56
1.58
1.58
Cascade
F2
0.379
0.146
0.214
0.229
A2
0.176
0.039
0.063
0.061
2
fl•
0.55,q
0.593
0.558
0.527
Estimatedflux and areacascade
parameters
for severalflights.
16,194
KER]V[AN AND BERNIER:
MULTIFRACTAL
BREAKING
WAVES
direct energy input from the wind, transfer to neigh- Conclusions
boring wavenumbers,and direct dissipation. The order
of magnitude of each term in the spectralbalancewas
An image of a field of breakingwaveson the ocean
given by
surface itself contains two well-defined subprocesses'
the reflective,low-intensity,nonbreakingRayleighback3
1
• --* u,ak
-• --* u,A
(26) groundand the scattered,moreintensefoam and white-
caps constitutinga fractal process. Their separation
In (26), k is the wavenumber
and u. is the friction within the image is relatively easily achievedusing a
velocityassociatedwith the (predominant)fractionof signal to noise ratio based on the ratio of the meathe integratedmomentumflux, whichlocally variesas sured cumulative probability function to an empirical
Rayleighdistributionbasedon the bulk (90%)of the
r --• u.ak
-3/2 --•
image.
The thresholdintensity aboveis connectedin isolated
islands
whoseindividual pixels, without regard for their
For our purposeswe have reinterpreted radial waveconnectedness,demonstrate a statistical invariance to
length when squaredas an area A and havethus passed
averagingindicative of a fractal process.When
from a local spectral representationto a local spatial spatial
these islands are connected into subsets and the islands
representation.
reordered by their singularity strength a, defined in
of Mandelbrot[1974],Frischel ai. [1978],Schertzerand terms of their fractional contributionto the total light
and area of the set above threshold, the accumulation of
Lovejoy[1984, 1987], and Meneveauand $reenivasan
light and area is smooth. This contraststo the 'devil's
The fractal casacademodelis similar in spirit to those
[1987b]in characterizing
intermittencyand turbulence. staircase'
Considera BC processwhich conservesan appropriate
flux F (e.g. energy,momentum)with successive
partitions from a mother interval, representingarea on the
surface,to two subintervalor daughterareas. Consider
a fraction fi of the flux from the previousstagecarried
to the surviving daughter intervals of nontrivial fractional area ai. Successive
iterationsonto the surviving
subregions
lead to a uniquerealization,eachfor a given
random set of permutations, to establish the relative
placementat each stage. The final result of many iterationsis a division of the original flux onto highly
localizedregions,in fact, the supportof the dissipative
process.
The generalizedBC processdescriptioncontainsfour
variables(fi and ai(i -- 1,2)) and the constraintthat
the flux is conserved.We are motivated by Phillips's
argumentsfor energy (and possiblyequivalentlymomentum) flux as a function of scaleto proposethat
the fractionalfluxesand receivingareasfrom onestage
of the partition processto the next are related. We
accordingly
proposea generalization
(26), that is,
- a,
The representationis somewhatmore generalthan
wouldresultfrom the arguments
of Phillips(•/i = 1),
structure
that
would
occur had the islands
been summedas encountered,say, by scanningorthogonally accordingto the axesof the image. The process
in effect producesthe smoothestacumulation function
possiblebasedon the Lipschitzconditionimplicit in the
definitionof the singularitystrength(21).
A closer examination
of the relative
accumulation
of brightnessand size demonstratesthat for small a,
light accumulatesfaster than area. It was argued that
this result
can be attributed
to those connected
sub-
sets in which the entrainment processleads to an increased vertical
extent of bubbles and hence more mul-
tiple light scattering. Converselythe runout stage of
breaking wavesin which the vertical extent is confined
to the interface,has reducedmultiple-scatteringopportunities. As well, it containsholeswhere the scattering
is nonexistentand therefore,will make a larger contribution to apparent area and a smaller contribution to
light. This conclusionis consistentwith the often-cited
divisioninto active(whitecap)and passive(foam)contributions to the total extent of breaking waves.
The predicted split between active entrainment and
passivefoam usinga critical c•c- i drawnfrom a point
of balancebetweenthesetendenciesagreeswell with existing estimatesbasedon an examination of the intensity abovethresholdin individual photographsor video
records based on the concept of a critical reflectivity
to separate foam from whitecaps. Additional study is
requiredto better achievethe basicfractal/nonfractal
separationof the image elements.
The analysis in the Fractal Spectrum section has
shownthat spatial distributionof breakingwaveson the
as it allows for two different subprocesses
to coexist
throughout the iterated partition operation. It is also
similar in spirit to classicalturbulence closureswhich
relate energeticsand fluxes to scale.
What is most remarkable in Table 2 is the very limited range of •/i over the differentflights. The standard
Proof of this contention
deviation of estimatescomparedto their averagevalue ocean surface is multifractal.
is 4 and 0.6% for i=l,2. Their consistency,
in view of followsfrom the power law structure of the estimatesof
the number of degreesof freedom,leadsus to conclude various moments between 4 and -2 as a function of the
tentatively that the observedimagesare well described spatial scaleof the averaging.It appearsthat the agreeby a BC processand that the parameterizationlinking ment has been disturbed by the presenceof swell and
the flux fraction to the areal subdivision is invariant to
the limited digital precisionin the positive and negathe wind speed and fetch.
tive moment estimations,respectively.The significance
KERMAN AND BERNIER: MULTIFRACTAL
of the main conclusionof this paper, that the breaking wave field is indeed multifractal, lies beyond the
relatively simple description of the obvious statistical
geometry.Classicalmodelsof forcingof the seasurface
have not includedintermittencyuntil recently [Glazman, 1986; $hen and Mei, 1993]. The contributionof
this work is that the centersof dissipation,the breaking
waves, are clearly multifractal. Despite such assumptions in models, no measurementsexist as to whether
the centersof energyinput from the wind are alsofractal. A useful study would therefore attempt to link the
centersof energyinput and dissipation.A model which
essentiallyassumesthat the centers are indistinguishable has been presented. It is based on the simplest,
nontrivial representation of the whitecapping process
in the form of a Besicovitch-Cantorfractal generator.
Preliminary analysisindicatesthat two subprocesses
exist that maintain a fixed relationship between flux and
area. This parameterization is similar in spirit to classical turbulence closureapproximations. The subprocess
carrying the majority of the flux apparently increases
with increaseswith wind speed. However, the limited
rangeof wind speedand the rather coarseimageresolution necessarilyweaken our conclusions. It remains to
repeat the experiment with finer spatial resolution imagery,directly measuredinsitu near-surfacewinds and
fluxes, and refined data processing.
Acknowledgments.
The authors would like to thank
Shaun Lovejoy for his suggestionto examine the imagery
for its possiblemultifractal structure. The work has benefited from the interest of many colleaguesat the University
of Cambridge, the Atmospheric Environment Service, the
Canada Centre for Inland Waters, and elsewhere, and we
wish to thank
them.
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(Received
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October
11,1993;
acceptedJanuary 7, 1994.)