Annu. Rev. Fluid Mech. 1999. 31:417–57
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A NEW VIEW OF NONLINEAR
WATER WAVES: The Hilbert Spectrum1
Norden E. Huang1, Zheng Shen2, and Steven R. Long3
1Division
of Engineering Science, California Institute of Technology, Pasadena,
California 91125. On leave from Laboratory for Hydrospheric Processes, Oceans
and Ice Branch, Code 971, NASA Goddard Space Flight Center, Greenbelt,
Maryland 20771
2Division
of Engineering Science, California Institute of Technology, Pasadena,
California 91125 and Department of Civil Engineering, University of California at
Irvine, Irvine, California 92697
3Laboratory for Hydrospheric Processes, Observational Science Branch, Code 972,
NASA GSFC, Wallops Flight Facility, Wallops Island, Virginia 23337;
e-mail:
[email protected]
KEY WORDS:
Hilbert transform, Hilbert spectral analysis, empirical mode decomposition,
nonlinear process, nonstationary
ABSTRACT
We survey the newly developed Hilbert spectral analysis method and its applications to Stokes waves, nonlinear wave evolution processes, the spectral form
of the random wave field, and turbulence. Our emphasis is on the inadequacy of
presently available methods in nonlinear and nonstationary data analysis. Hilbert
spectral analysis is here proposed as an alternative. This new method provides
not only a more precise definition of particular events in time-frequency space
than wavelet analysis, but also more physically meaningful interpretations of the
underlying dynamic processes.
INTRODUCTION
Historically, there are two views of nonlinear mechanics: the Fourier and the
Poincaré. The traditional Fourier view is an outcome of perturbation analysis in
1 The US government has the right to retain a non-exclusive, royalty-free license in and to any
copyright covering this paper.
417
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HUANG ET AL
which a nonlinear equation is reduced to a system of linear ones. The final solution becomes the sum of these linear equations. In most mechanics problems,
the linearized equations are second order; therefore, the solutions are trigonometric functions, and the sum of the solutions of this linear system constitutes
the Fourier expansion of the “true” solution. This is thus the Fourier view: The
system has a fundamental oscillation (the first-order solution) and bounded
harmonics (all the higher-order solutions). Although this approach might be
mathematically sound, and seems to be logical, the limitations of this view become increasingly clear on closer examination: First, the perturbation approach
is limited to only small nonlinearity; when the nonlinear terms become finite,
the perturbation approach then fails; Second, and more importantly, the solution obtained makes little physical sense. It is easily seen that the properties
of a nonlinear equation should be different from a collection of linear ones;
therefore, the two sets of solutions from the original equation and the perturbed
ones should have different physical and mathematical properties. Realizing this
limitation, recent investigators of nonlinear mechanics adopted a different view,
that of Poincaré.
Poincaré’s system provides a discrete description. It defines the mapping
of the phase space onto itself. In many cases, Poincaré mapping enables a
graphical presentation of the dynamics. Typically, the full nonlinear solution is
computed numerically. Then the dynamics are viewed through the intersections
of the trajectory and a plane cutting through the path in the phase space. The
intersections of the path and the plane are examined to reveal the dynamical
characteristics. This approach also has limitations, for it relies heavily on the
periodicity of the processes. The motion between the Poincaré cuts could also
be just as important for the dynamics. Both the Fourier and Poincaré views have
existed for a long time. Only recently has an alternative view for mechanics,
the Hilbert view, been proposed.
The Hilbert view is based on a new method, called empirical mode decomposition (EMD) and Hilbert spectral analysis as described by Huang (1996)
and Huang et al (1996, 1998a). It has found many immediate applications in
a variety of problems covering geophysical (Huang et al 1996, 1998a) and
biomedical engineering (Huang et al 1998b). In this review, the new method
will be summarized, and fluid mechanics examples of nonlinear water waves
and turbulence data will be used to illustrate the use of this method to interprete
the dynamics of these phenomena.
As the new method became available only recently, it is necessary to give
a summary of it and describe some recent improvements to it here. Huang
et al (1998a) clearly point out that a faithful representation of the nonlinear and
nonstationary data requires an approach that differs from Fourier or Fourierbased wavelet analysis. The new method developed by Huang et al (1998a)
seems to fit this need. This method uses two steps to analyze the data. The
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NONLINEAR WAVES: THE HILBERT SPECTRUM
419
first step is to decompose the data according to their intrinsic characteristic
scales into a number of intrinsic mode function (IMF) components by using
the empirical mode decomposition method. In this way, the data are expanded
in a basis derived from the data itself. The second step is to apply the Hilbert
transform to the IMF components and construct the time-frequency-energy
distribution, designated as the Hilbert spectrum. In this form, the time localities
of events will be preserved, for frequency and energy defined by the Hilbert
transform have intrinsic physical meaning at any point. We will introduce the
whole process by starting from the Hilbert transform.
THE HILBERT TRANSFORM
For an arbitrary time series, X (t), we can always have its Hilbert transform,
Y (t), as
Z
X (t ′ ) ′
1
dt ,
(1)
Y (t) = P
π
t − t′
where P indicates the Cauchy principal value. This transform exists for all
functions of class Lp (see, for example, Titchmarsh 1948). With this definition,
X (t) and Y (t) form a complex conjugate pair, so we can have an analytic signal,
Z (t), as
Z (t) = X (t) + Y (t) = a(t)eiθ (t) ,
(2)
in which
1
a(t) = [X 2 (t) + Y 2 (t)] 2 ;
(3)
Y (t)
.
X (t)
Theoretically, there are an infinite number of ways to define the imaginary
part, but the Hilbert transform provides a unique way for the result to be an
analytic function. A brief tutorial on the Hilbert transform, with emphasis on its
physical interpretation, can be found in Bendat & Piersol (1986). Essentially,
Equation (1) defines the Hilbert transform as the convolution of X (t) with 1/t;
therefore, it emphasizes the local properties of X (t). In Equation (2), the polar
coordinate expression further clarifies the local nature of this representation: it
is the best local fit of an amplitude- and phase-varying trigonometric function
to X (t). Even with the Hilbert transform, there is still considerable controversy
in defining the instantaneous frequency as
dθ(t)
.
(4)
ω(t) =
dt
Detailed discussions and justifications are given by Huang et al (1998a). With
this definition of instantaneous frequency, its value changes from point to point
θ(t) = arctan
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HUANG ET AL
in time. Two simple examples in Figure 1 (see color figure at end of volume) illustrate this approach. Figure 1a gives the familiar sine wave changing from one
frequency to another. These data are certainly nonstationary, a characteristic
that repeatedly demonstrates the power of wavelet analysis. The wavelet spectrum in color and the Hilbert analysis representation as a thin line through the
wavelet spectrum are shown in Figure 1b. Their projections on the frequencyenergy plane are shown in Figure 1c. The comparison is clear: The Hilbert
representation gives a much sharper resolution in frequency and a more precise
location in time. The second example is the common exponentially damped
oscillation. The data, wavelet and Hilbert representations, and their projections
are given in Figures 1d–f, respectively. Again, it can be seen that the Hilbert
representation gives a superior resolution in time and frequency. Based on these
comparisons, we can conclude that wavelet analysis indeed improves the time
resolution compared with the Fourier method. Wavelet analysis gives a uniform
frequency resolution, but as can be seen, the resolution is also uniformly poor.
Convenient and powerful as the Hilbert transform seems, by itself it is not
usable for general random data, as discussed by Huang et al (1998a). In the
past, applications of the Hilbert transform have been limited to narrow band
data; otherwise, the results are only approximately correct (Long et al 1993b).
Even under such restrictions, the Hilbert transform has been used by Huang
et al (1992) and Huang et al (1993) to examine the local properties of ocean
waves with detail that no other method has ever achieved. Later, it was also used
by Huang (1995) to study nonlinear wave evolution. For general application,
however, it is now obvious that the data will have to be decomposed first, as
proposed by Huang et al (1998a).
Independently, the Hilbert transform has also been applied to study vibration
problems for damage identification (Feldman 1991, 1994a,b, Feldman & Braun
1995, Braun & Feldman 1997, and Feldman 1997). In all these studies, the
signals were limited to “monocomponent” signals, i.e. without riding waves.
Furthermore, the signals have to be symmetrical with respect to the zero mean.
Thus, the method is limited to simple, free vibrations. Although Prime &
Shevitz (1996) and Feldman (1997) have used it to identify some of the nonlinear
characteristics through the frequency modulation in a nonlinear structure, the
limitation of the data renders the method of little practical application in both
identifying and locating the damage. The real value of the Hilbert transform had
to wait to be demonstrated until Huang et al (1998a) introduced the empirical
mode decomposition (EMD) method, which is based on the characteristic scale
separation. The EMD method was developed to first operate on the data being
processed and to then prepare it for the Hilbert transform. Therefore, we will
discuss the time scale problem next, since this concept is central to this new
approach.
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Figure 1 Comparisons of Wavelet and Hilbert representation for simple symmetric data. The Hilbert transform
can be applied to these types of data to give better time-frequency resolution without difficulty.
NONLINEAR WAVES: THE HILBERT SPECTRUM
421
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THE CHARACTERISTIC SCALES
According to Drazin (1992), the first method of time series analysis is inspection
by eye. This approach is, of course, subjective. But a trained eye can detect
many trends and patterns of the data that are hard to quantify. Even to the
untrained eye, there are certain properties of the data that are easy to pick up.
Let us take, for example, the stationarity, the periodicity, the overall trend,
and various scales defined by the time lapses between specific types of points.
Valuable as these insights are, inspection by the eye alone is too subjective to
be of any serious use. Of the various quantities the eye can pick up, the time
scale is one that can be quantified most easily.
In interpretation of any physical data, the most important parameters are the
time scale and the energy distribution with respect to it. There is no difficulty
in defining the local energy density, but up until now, no clear definition of the
local time scale has ever been given. In Fourier analysis, the time scales are
defined as the periods of the continuous and constant-amplitude trigonometric
components. As discussed in Huang et al (1998a), such a definition gives only
a global averaged meaning to the energy and time scales. As such, these scales
are totally divorced from the reality of time variations of either the amplitude
or the frequency.
Statistical definitions of the time scale have been made by Rice (1944, 1945),
who computed the expected numbers of zero-crossings, and the extrema for any
data under linear, stationary, and normal distributed assumptions. Mathematically, the time scales are defined for any data, x(t), as follows: The locations
of t for
x(t) = 0
(5)
are defined as the points of zero-crossings. The time spacing between successive
zero-crossing is the zero-crossing time scale. The locations of t for
Ẋ (t) = 0
(6)
are defined as the points of the extrema. The time spacing between successive
extrema is the extrema time scale.
Under the linear, stationary, and normal distribution assumptions, the expected number of zero-crossings and the expected number of extrema can be
computed from Rice’s formulae. But those definitions offer only a global measure, which cannot be applied to real nonlinear and nonstationary data. Because
of the limitations set forth in Rice’s assumptions, his results have also created
a paradox: in many data, the number of expected extrema computed from his
formula becomes unbounded. If most data are linear and stationary, then why
can we not apply the formula to them? This is because the Fourier power spectra usually have asymptotic power law forms. For example, if the spectrum has
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HUANG ET AL
a −3 power law, then m2 is unbounded. For a white noise or a delta function,
the spectrum is white and then even the zero-crossing is undefined. Take ocean
wave data as an example. The asymptotic form of the frequency spectrum has a
power law form with the power between −4 and −5 (see, for example, Phillips
1958, Toba 1973, Phillips 1977, Kitaigorodskii 1983, Banner 1990, Belcher
& Vassilicos 1987). Then, according to Rice’s formula, the expected number
of extrema is unbounded. Yet we can certainly count the extrema without any
difficulty. This dilemma, however, has not yet caused most investigators to
question the formulae and the assumptions involved, but it has led them to reject any formula that involves moments higher than the 4th. Such an approach
has limited the statistical measure of time scales to the computation of the zerocrossings only. Hence the statistics of the zero-crossings are too crude to be of
any real use.
The spacing of the extrema certainly offers a better measure of time scale,
because this approach can measure wide-band data with multiple riding waves.
It certainly agrees with our intuition of the time variations of the data. Refined
as the extrema criterion is, it is not always precise enough. If one examines
the data more closely, one will find that even the spacing of the extrema can
miss some subtle time-scale variations, because there are weak oscillations
that can cause a local change in curvature but not create a local extremum, a
phenomenon known as hidden scales. To account for this type of weak signal,
we introduce still another type of time scale based on the variation of curvature.
Mathematically, this is equivalent to finding extreme values of
Ẍ
.
(6a)
2 3
(1 + Ẋ ) 2
Dynamically, the curvature is equivalent to the measure of the weighted acceleration. Any change of sign of the curvature indicates a change of the sign of
the force. As such, the curvature variation indeed has strong dynamic significance. As we see, if the extrema statistics have already encountered difficulties
in models, the extreme values of the curvature would involve the 8th moment of
the spectrum from the data. Trying to compute it under the linear and stationary assumption is impossible. Fortunately, this difficulty is but a mathematical
artifact, a consequence of the linear and stationary assumptions invoked. We
certainly can compute the curvature and its extrema, and then count them.
Consequently, the failure of Rice’s formulae is another indication of what we
believe to be the falsehood of the commonly invoked assumptions of linearity
and stationarity.
We now have three methods of measuring the time scales: the time between
successive zero-crossings, the time between successive extrema, and the time
between successive curvature extrema. In each case, the time span is a local
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NONLINEAR WAVES: THE HILBERT SPECTRUM
423
measure of the time variation of events. In the case of extrema and curvature
spans, the local time scale counts all the waves, whether they cross the zero line
or not. The aim is to define a local time scale of oscillation that will change
from one extreme (by the restoring force through the zero point) to the other
extreme of the opposite sign. This is the characteristic time scale. It is local,
and it represents only one mode of oscillation. So we regard it as the intrinsic
scale of the oscillation.
Zero-crossing is a very crude measure of the data. Unless the data are truly
narrow band, there might be many extrema between two consecutive zerocrossings. Our eyes are much more sensitive to the variations of the spacing
between extrema, and these variations offer a more detailed measure of the
given phenomena. Yet the time lapses between extrema have been problematic. The fourth moments for many phenomena are not convergent, so the expected number of extrema is impossible to compute, even though it might be
easily counted. This paradox is easily resolved by considering a bold concept:
The Fourier power-law spectra of most data are artificial. Most of the highfrequency components are from the spurious harmonics from either nonlinearity
(singular points, such as corners, and cusps in the data train), or nonstationarity.
Following Huang et al (1998a), the time scale between extrema is the key and
therefore will be used as the time scale in the decomposition.
THE EMPIRICAL MODE DECOMPOSITION METHOD:
THE SIFTING PROCESS
As discussed by Huang et al (1996, 1998a), the empirical mode decomposition
method is necessary to deal with both nonstationary and nonlinear data. Unlike
almost all the previous methods, this new method is intuitive, direct, a posteriori,
and adaptive, with the basis of the decomposition being derived from the data.
The decomposition is developed from the simple assumption that any data
consist of different simple intrinsic modes of oscillations. Each mode may or
may not be linear, and will have the same number of extrema and zero-crossings.
Furthermore, the oscillation will also be symmetric with respect to the “local
mean.” The term local mean is an oxymoron. Any mean will involve a time
scale to define it. Here, however, the mean is defined through the envelopes
without resorting to any time scale. (Its precise definition is given below.) With
this definition of local mean, modes of different time scales can be separated
by their characteristic scales, defined as the time lapses between the successive
extrema. At any given time, there might be many different coexisting modes of
oscillation, each superimposed on the others. The final complicated data results.
Once separated, each mode should be independent of the others; they have no
multiple extrema between successive zero-crossings. Thus each is designated
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as an intrinsic mode function (IMF) by the following definitions: (a) in the
whole data set, the number of extrema and the number of zero-crossings must
either equal or differ at most by one; and (b) at any point, the mean value of
the envelope defined by the local maxima and the envelope defined by the local
minima is zero.
An IMF represents a simple oscillatory mode as a counterpart to the simple
harmonic function, but it is much more general. With the definition, one can
decompose any function as follows: (a) Identify all the local extrema, then
connect all the local maxima by a cubic spline line as the upper envelope;
(b) Repeat the procedure for the local minima to produce the lower envelope.
The upper and lower envelopes should cover all the data between them. Their
mean is designated as m 1 , and the difference between the data and m 1 is the
first component, h 1 , i.e.
X (t) − m 1 = h 1 .
(7)
The procedure is illustrated in Huang et al (1998a).
Ideally, h 1 should be an IMF, for the construction of h 1 described above
should have required it to satisfy all the requirements of an IMF. Yet, even if
the fitting is perfect, a gentle hump on a slope can be amplified to become a
local extremum in changing the local zero from a rectangular to a curvilinear
coordinate system. After the first round of sifting, the hump may become a
local maximum. New extrema generated in this way recover the proper modes
lost in the initial examination. In fact, the sifting process can recover signals
representing low-amplitude riding waves with repeated siftings.
The sifting process serves two purposes: to eliminate riding waves, and to
make the wave profiles more symmetric. While the first condition is absolutely
necessary for separating the intrinsic modes and for defining a meaningful
instantaneous frequency, the second condition is also necessary in case the
neighboring wave amplitudes have too large a disparity. Toward these ends,
the sifting process has to be repeated as many times as is required to reduce the
extracted signal to an IMF. In the subsequent sifting process steps, h 1 is treated
as the data; then
h 1 − m 11 = h 11 .
(8)
After repeated sifting, i.e. up to k times, h 1k becomes an IMF, that is
h 1(k−1) − m 1k = h 1k ;
(9)
then it is designated as
c1 = h 1k ,
the first IMF component from the data.
(10)
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NONLINEAR WAVES: THE HILBERT SPECTRUM
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As described above, the process is indeed like sifting: to separate the finest
local mode from the data first, based only on the characteristic time scale. To
guarantee that the IMF components retain enough physical sense of both amplitude and frequency modulations, the number of times the sifting process repeats
has to be limited. Too many sifting cycles could reduce all components to a
constant-amplitude signal with frequency modulation only. Then, the components would lose all their physical significance. A simple criterion for stoppage
is when the number of extrema equals the number of zero-crossings. The
original Cauchy-like convergence criterion introduced by Huang et al (1998a)
should be used with great care, because the deviations between successive
siftings are controlled primarily by the appearance of new extrema from their
previously hidden state. Such problems can be resolved now with curvature
sifting. Therefore, the criterion for stoppage can be simplified, as proposed
here.
Overall, c1 should contain the finest scale or the shortest period component
of the signal. We can separate c1 from the rest of the data by
X (t) − c1 = r1 .
(11)
Since the residue r1 still contains longer-period components, it is treated as the
new data and subjected to the same sifting process as described above. This
procedure can be repeated for all the subsequent r j ’s, and the result is
r 1 − c2 = r 2 ,
···
(12)
rn−1 − cn = rn
The sifting process can be stopped by any of the following predetermined
criteria: either when the component cn or the residue rn becomes so small that
it is less than the predetermined value of substantial consequence, or when the
residue rn becomes a monotonic function from which no more IMF can be
extracted. Even for data with zero mean, the final residue still can be different
from zero. If the data have a trend, the final residue should be that trend. By
summing up Equations (11) and (12), we finally obtain
X (t) =
n
X
c j + rn .
(13)
j=1
Thus, one can achieve a decomposition of the data into n-empirical modes, and
a residue rn , which can be either the mean trend or a constant. As discussed
here, to apply the EMD method, a mean or zero reference is not required; EMD
needs only the locations of the local extrema. The zero references for each
component will be generated by the sifting process. Without the need of the
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HUANG ET AL
zero reference, EMD avoids the troublesome step of removing the mean values
for the large DC term in data with non-zero mean, an unexpected benefit.
To illustrate the sifting process, we will use a set of length-of-the-day data
covering the period from 1978 to 1988. The data are given in Figure 2a. Clearly,
the data are quite complicated, with many local extrema but no zero-crossings,
because the time series represents all positive numbers. Although the mean
can be treated as a zero reference, defining it is hard, for the whole process
is transient. This example illustrates the advantage of adopting the successive
extrema for defining the time scale; it also illustrates the difficulties of dealing
with nonstationary data: Even a meaningful mean is impossible to define, but
for the EMD method, this difficulty is eliminated. Figure 2b summarizes all the
IMFs obtained from this repeated sifting process. Figure 2b illustrates a total
of 7 components plus a residue term. In comparison to the traditional Fourier
expansion, one can immediately see the efficiency of EMD.
The components of EMD are usually physical, for the characteristic scales
are physical. In Figure 2b, we can see the yearly cycle clearly as the fifth component C5. The first two are semi-monthly and monthly tidal modulation of the
rotation speed of the earth. Different from the Fourier analysis, each component still retains both frequency and amplitude modulations. For example, the
amplitude of the annual fluctuation is slightly larger at 1982, which happens to
be an unusually strong El Niño year.
To demonstrate the completeness of the decomposition, the IMF components
can be added back one by one to form the original data. Figure 3a shows the
data in a dotted line and the residue term in a solid line. By itself, the residue
is not an impressive running mean of the data. It should not be, for the last
IMF is not a mean; it is only the residue after all the oscillatory terms have
been separated from the signal. In this sense, it could be a trend. By adding the
longest period IMF component, the sum gives a sense of a much better running
mean, as in Figure 3b. The third component gives the annual cycle. The sum
immediately shows the fluctuation of the length of the day by year in Figure 3d.
By successively adding all the components, we eventually get Figure 3h, which
is indistinguishable from the original data. The numerical difference between
the sum of the IMFs and the original data is given in Figure 3i. The magnitude
is only of the order of 10−15 . It is the round-off error for the computer. Thus,
the completeness of the expansion is proven numerically.
To use the unique definition of instantaneous frequency, we have to reduce an
arbitrary data set into IMF components from which an instantaneous frequency
value can be assigned to each IMF component. Consequently, for complicated
data, we can have more than one instantaneous frequency at a time locally. After
decomposing the data into IMFs, and after operating on these with the Hilbert
transform, we can then present the result, which we call the Hilbert spectrum.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
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Figure 2 Demonstration of the empirical mode decomposition method from length-of-the-day deviation data; the unit is microseconds.
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HUANG ET AL
Figure 3 Reconstruction of the original data from the IMF components. The difference between
the reconstructed and the original data is only 10−9 microsecond.
Intermittency Test
The sifting process described above seems straightforward. Yet straightforward
application of the sifting method may run into difficulties when the data contain
intermittency, which will cause mode mixing. We discuss this phenomenon in
more detail below.
Let us consider the data given in Figure 4a, where there is a train of largeamplitude sine waves with another train of small-amplitude sine waves occurring intermittently. With application of the straightforward sifting, we will
obtain the components as shown in Figure 4e–h, in which the first two IMF
components contain seriously mixed modes, that is, modes of very different
periods. Take the component in 4e as an example. The small wave train is
clearly identified. Wherever the small waves are identified, the underlying
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NONLINEAR WAVES: THE HILBERT SPECTRUM
429
Figure 4 Effect of intermittency criterion in the EMD sifting process invoked to eliminate mode
mixing. Sequence b–d with intermittency check; sequence e–h without intermittency check.
large waves will not be included in this IMF component. On the other hand,
wherever there is no small-wave component, the large waves are retained as
part of the component. As a result, there is a great disparity in the periods of
the first IMF component. This is mode mixing; it is caused by intermittency
occurring in part of the signal.
To overcome the mode mixing, a criterion based on the period length is
introduced to separate the waves of different periods into different modes. The
criterion is set as the upper limit of the period that can be included in any given
IMF component. With this criterion introduced, the result is shown in Figure
4b–d. Clearly, the intermittent small wave was separated from the large waves.
Any additional criterion introduced in the sifting process implies an intervention with a subjective condition. Such intervention could cause severe bias
in the final result; therefore, the introduction of any additional condition should
be justified with clear and strong arguments. As a rule, data should be processed first without any added conditions. The intermittency criterion should
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HUANG ET AL
be introduced only when the sifted results clearly show the problem of mode
mixing. Mode mixing cannot be justified from physical grounds, for any oscillator cannot have great disparity in its periods.
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THE HILBERT SPECTRUM
Having obtained the intrinsic mode function (IMF) components, one will have
no difficulty in applying the Hilbert transform to each of these IMF components
and computing the instantaneous frequency according to Equation (4). After
performing the Hilbert transform to each IMF component, the original data can
be expressed as the real part (RP) in the following form:
n
R
X
X (t) = R P
a j (t)ei ω j (t)dt .
(14)
j=1
Here we have left out the residue rn on purpose, for it is either a monotonic
function or a constant. Although the Hilbert transform can treat the monotonic
trend as part of a longer oscillation, the energy involved in the residual trend
could be overpowering. In consideration of the uncertainty of the longer trend,
and in the interest of information contained in the other low-energy but clearly
oscillatory components, the final non-IMF component should be left out. It
could be included, however, if physical considerations justify its inclusion.
Equation (14) gives both amplitude and frequency of each component as
functions of time. The same data, if expanded in the Fourier representation,
would be
X (t) = R P
∞
X
a j eiω j t ,
(15)
j=1
with both a j and ω j constants. The contrast between Equations (14) and (15)
is clear: the IMF represents a generalized Fourier expansion. The variable
amplitude and the instantaneous frequency have not only greatly improved the
efficiency of the expansion, but also enabled the expansion to accommodate
nonstationary data. With the IMF expansion, the amplitude and the frequency
modulations are also clearly separated. Thus, we have broken through the restriction of the constant amplitude and fixed frequency imposed by the Fourier
expansion, and arrived at a variable amplitude and frequency representation.
Now let us illustrate the difference between the two expressions graphically
in the frequency-energy-time space. Figure 5a (see color figure at end of
volume) represents a set of highly transient data. In the Fourier expansion,
the frequency and amplitude are not time dependent; therefore, all Fourier
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Figure 5 The comparison of Hilbert and Fourier spactral analysis for highly transient data. The Fourier
method cannot reveal of the variation of the signal with time.
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Figure 6 The Hilbert and marginal spectra for the length of the day data. It gives detailed time variation of
the frequency with time.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
431
components are represented by rectangular blocks with thickness of dω, as in
Figure 5c. Consequently, the only information is the projection of the blocks on
the frequency-energy plane. This is why the Fourier spectra can be meaningful
only for stationary data. The same data, if expanded in terms of IMF, will
produce the result as given in Figure 5b. As the frequency of each component
is a function of time, it is a curve on the time-frequency plane. Furthermore,
because the amplitude (or the energy) of each component is also a function of
time, the final energy representation is a curve in the three-dimensional space
of frequency-energy-time. This frequency-time distribution of the amplitude
is designated as the Hilbert amplitude spectrum H (ω, t), or simply the Hilbert
spectrum. If amplitude squared is preferred to represent energy density, then
the squared values of amplitude can be substituted to produce the Hilbert energy
spectrum just as well.
Various forms of the Hilbert spectra presentations can be made: color-coded
maps and contour maps all with or without smoothing. The Hilbert spectrum
in the color map format for the length-of-the-day data is given in Figure 6a
(see color figure at end). The Hilbert spectrum appears only in the skeleton (or
line) form with emphasis on the frequency variations of each IMF, while the
wavelet analysis result usually gives a smoothed energy contour map with a rich
distribution of higher harmonics. The skeleton presentation is more desirable,
because it gives more quantitative results. Bacry et al (1991) have tried to extract
the wavelet skeleton as the local maximum of the wavelet coefficient, but even
that approach is encumbered by the harmonics. If more qualitative results are
desired, a fuzzy view can also be derived from the skeleton presentation by using
two-dimensional smoothing. We will discuss the significance of the difference
between the Hilbert and wavelet presentations further on in this review.
With the Hilbert spectrum defined, we can also define the marginal spectrum,
h(ω), as
Z T
H (ω, t)dt.
(16)
h(ω) =
0
The marginal spectrum offers a measure of the total amplitude (or energy)
contribution from each frequency value. It represents the cumulated amplitude
over the entire data span in a probabilistic sense. In Figures 5d and 6b, the
solid lines give the corresponding marginal spectrum of the Hilbert spectrum
given in Figures 5b and Figure 6a, respectively. The lack of harmonics is clearly
demonstrated. Furthermore, Figure 5d showed a much richer energy content in
the low-frequency range than the corresponding Fourier spectrum in Figure 5e.
This is usually the case, for the constant amplitude and frequency Fourier
representation would never be able to depict the true energy content. It should
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432
HUANG ET AL
be pointed out that the marginal spectra should not be used for any nonstationary
data, for the marginal spectra are the projections rather than the substance of
the real frequency-energy-time distribution.
As pointed out by Huang et al (1996), the frequency in either h(ω, t) or
h(ω) has a totally different meaning from the Fourier spectral analysis. In
the Fourier representation, the existence of energy at a frequency ω means that
a component of a sine or a cosine wave persisted through the time span of
the data. Here, the existence of energy at the frequency ω means only that
in the whole time span of the data, there is a higher likelihood for such a
wave to have appeared locally. In fact, the Hilbert spectrum is a weighted nonnormalized joint amplitude-frequency-time distribution. The weight assigned
to each time-frequency cell is the local amplitude. Consequently, the frequency
in the marginal spectrum indicates only that the likelihood of an oscillation with
such a frequency exists. The exact time of that oscillation is given in the full
Hilbert spectrum.
Having defined the Hilbert spectrum, we thus have a real frequency-energytime representation of the data that is quantitative. With it, Huang et al (1998a)
have defined the degree of stationarity (DS) as
¶
Z µ
H (ω, t) 2
1 T
1−
dt.
(17)
DS(ω) =
T 0
h(ω)/T
This definition of degree of stationarity is very similar to the intermittency
used in the wavelet analysis proposed by Farge (1992). A degree of statistical
stationarity is also defined by Huang et al (1998a). The instantaneous energy,
IE, can also be defined as
Z
IE(t) =
H 2 (ω, t)dω.
(18)
ω
VALIDATION AND CALIBRATION
OF THE HILBERT SPECTRUM
Through empirical mode decomposition and the associated Hilbert spectral
analysis, we obtained the probabilistic Hilbert spectrum representation of the
nonlinear and nonstationary data. Now we will validate the approach and the
results, and calibrate its fidelity against the best existing method, wavelet
analysis.
Let us first consider the following mathematical model:
X (t) = cos(ωt + ε sin 2ωt).
(19)
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Figure 7 Camparison of Hilbert and Wavelet spectra for the intra-wave modulation case.
The Hilbert view avoids the harmonics, and it gives the real intra-wave frequency modulations.
NONLINEAR WAVES: THE HILBERT SPECTRUM
433
According to the classic wave theory, this expression is a clear case of intra-wave
frequency modulation. The frequency, , at any time is simply
= ω(1 + 2ε cos 2ωt).
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Yet from Equation (19), it is easy to show that
¶
µ
1
ε
cos ωt + cos 3ωt + . . . ,
X (t) = 1 −
2
2
(20)
(21)
which is similar to the second-order approximation of the Duffing equation
through perturbation analysis. The Hilbert and wavelet spectra for these are
given in Figure 7a (see color figure). Here we have two views for the same mathematical expression. Both representations can be used to construct the original
curve, but they convey very different physical meanings. Clearly, the one based
on classical wave theory is the more physical one, for it is how we define the
function. From this example, we can see that there are two types of frequency
modulations, inter-wave and intra-wave. The first type is familiar to us; the
frequency of the oscillation gradually changes as do the waves in a dispersive
system. Technically, in dispersive waves, the frequency also changes within
one wave, but that was not emphasized either for convenience, or for lack of a
more precise frequency definition. The second type is less familiar, but it is also
a common phenomenon: if the frequency changes from time to time within
a wave, its profile can no longer be described by simple trigonometric functions. Therefore, any wave profile deformation from the simple sinusoidal form
implies intra-wave frequency modulation. In the past, such phenomena were
treated as harmonic distortions. The purpose of the harmonics is not to represent the true frequency distribution, but rather to represent the waveform. The
marginal spectra of the Hilbert and wavelet spectra together with the Fourier
spectrum are shown in Figure 7b. Here the Hilbert spectrum clearly depicts the
modulation of the frequency as shown by Equation (19). Wavelet analysis again
gives a poor frequency resolution. Thus, we show in detail that most waveform
deformations are better viewed as intra-wave frequency modulations. This is
the core of the Hilbert view: it is more physical.
This simple example again illustrates that the instantaneous frequency, with
intra-wave frequency modulation defined by the EMD and Hilbert spectrum,
does make physical sense. In fact, such an instantaneous frequency presentation
reveals more details of the system: it reveals the variation of the frequency
within one period, a view never seen before.
The above examples have not only validated the EMD and the Hilbert spectrum representation, but also clarified the conditions under which spurious
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434
HUANG ET AL
harmonics are generated in Fourier-based analysis: nonlinearity and nonstationarity. In the past, this crucial problem has not been examined carefully.
Typically, perturbation analysis gives a solution in series expansion. Each term
is the solution of a linear equation. Although infinite series expansion is so powerful that it can approximate some transient phenomena with uniform amplitude
components, their physical meaning has never been examined critically. The
mathematical success has obscured our physical insights. With these idealized examples, we have established the validity and the limitations of Hilbert
spectral analysis. Next, we will present some applications in both numerically
computed results from low-dimensional nonlinear equations, and some data
from observations.
CLASSIC NONLINEAR SYSTEMS
The advantage of studying classic nonlinear systems is their simplicity, yet
they contain all the essentials of the possible nonlinear effects. All these systems have been studied extensively; therefore, although most of their dynamic
characteristics are familiar, their detailed physics may not be. We cite two examples: the Duffing equation and the Rössler equation, both used by Huang
et al (1998a).
The Duffing Equation
We use the classic Duffing equation to illustrate intra-wave frequency modulation. The Duffing equation is
d2x
+ x − εx 3 = b cos υt,
dt 2
(22)
in which ε is a small parameter. This equation can be written in a slightly
different form as
d2x
+ x(1 − εx 2 ) = b cos υt,
dt 2
(23)
where we have factored out x and (1 − εx 2 ). This equation can be viewed as a
nonlinear spring with a variable spring constant (1 − εx 2 ). If ε is zero, this is
a simple oscillator with constant period. If ε is not zero, the spring constant is
no longer a constant; it becomes a function of position. The period is longest
when the position is near the origin, and the shortest when the position is at the
maximum displacement. Thus, this nonlinear oscillator has variable frequency
within one cycle of oscillation. Clearly, this is a case of intra-wave frequency
modulation.
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Figure 9 The Hilbert and Marginal spectra for the Duffing equation solution. The Hilbert reveals the detailed
frequency modulation of the data.
NONLINEAR WAVES: THE HILBERT SPECTRUM
435
Traditionally, this problem has been treated by perturbation methods. If one
uses the straightforward perturbation method, one gets the secular term as
µ
¶
3
1
x(t) = cos t + ε
t sin t + (cos t − cos 3t) .
(24)
4
32
The homogeneous solution of Equation (22) is given in Drazin (1992) as
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x(t) = a cos ωt +
1 2
εa (cos ωt − cos 3ωt) + O(ε2 a 5 )
32
(25)
and
3
ω = 1 − εa 2 + O(ε 2 a 4 ) as ε → 0.
(26)
8
The above solutions work only for small ε. If we adopt the initial values
[x(0), x′ (0)] = [1, 1]; and a = 1, b = 0.1, ε = 1, υ = 1/25 Hz, we cannot use
the solution to evaluate the functional value of x anymore, for ε is now finite.
The full solution of Equation (22) subject to the initial conditions given here
has to be computed numerically. The numerical solution is given in Figure 8a.
The waveform is far from sinusoidal. All the deformations indicate nonlinear
effects, traditionally represented by harmonics. The full solution in the phase
plane is given in Figure 8b, and we see that the locus of the solution tends to
bunch into three distinguishable paths. This suggests that the motion within
this time period contains a period-three oscillation in addition to the forcing
function and the intrinsic oscillation time scales. These data, when subjected
to the empirical mode decomposition method, yield four components and a
residue, as shown in Figure 8c.
The first component is the intrinsic oscillation of the system subject to the
forcing, the second component is the forcing function, and the third component is the period time scale. All of these components are physical. With
these intrinsic mode functions, the Hilbert spectrum can be constructed as in
Figure 9a (see color figure) together with the original data. The most interesting component is the intrinsic oscillation term. In the Hilbert spectrum, it
is represented by an oscillatory line indicating the frequency change from one
instant to another. A detailed comparison between the Hilbert spectrum and the
data shows the uneven frequency variations from one wave to the next and is a
faithful and detailed representation of the fact that the motion has a different frequency within one oscillation. The intrinsic frequency shows strong intra-wave
frequency modulation, which is presented as a variable frequency oscillating
between 0.06 and 0.16 Hz, with a mean around 0.11 Hz, the averaged frequency
as predicted by the Hamiltonian method. The detailed variations of the intrinsic
frequency indicate that it contains both inter- and intra-wave frequency modulations. The forcing function is also clearly shown with the expected frequency.
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436
HUANG ET AL
Figure 8 Data, phase diagram, and IMF components for the solution of the Duffing equation.
Trajectories of motion show clear bunching at the preferred paths, indicating additional time scales.
The long-period component is the low-frequency and low-amplitude signal. It
represents the slow, aperiodic wobbling of the phase depicting the period-three
bunching of the paths. It is real. If we compute a longer time series, there will
be still longer-period motions. As the motion is already chaotic, the path may
never repeat itself.
A wavelet representation of the same data is given by Huang et al (1998a).
Because the Morlet wavelet used here is Fourier based, the variation of the
frequency has to be represented by harmonics. The marginal Hilbert spectra
together with the Fourier spectrum of the data are given in Figure 9b. Here, the
lack of harmonics in the Hilbert spectrum is clearly shown. This is a totally
different view of the nonlinear system. It tracks the instantaneous change of
the waveform by small changes of frequency rather than by using harmonics.
Although both the Fourier and the Hilbert representations show the same effect of waveform deformations, the physical meaning is very different: The
Hilbert representation gives a true physical interpretation of the dynamics by
NONLINEAR WAVES: THE HILBERT SPECTRUM
437
indicating the instantaneous value of the frequency, and thus the Hilbert view
is much more physical.
The Rössler Equation
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The nonlinear effect can also be represented by another classical example in
the Rössler equation as
dx
= −(y + z),
dt
dy
1
(27)
= x + y,
dt
5
dz
1
= + z(x − µ),
dt
5
in which µ is a constant parameter. The numerical value of x computed with
µ = 3.5 is given in Figure 10a with its phase diagram in Figure 10b. This is the
Figure 10 Data, phase diagram, and IMF components for the solution of the Rössler equation.
This is the case of period doubling, which indicates two time scales.
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438
HUANG ET AL
case of period doubling, when, starting from any point, one needs to spend twice
the simple oscillation time to return to the original state. Obviously, there must
be two time scales. The empirical mode decomposition method indeed gives
precisely two components and a numerically insignificant residual error term
in Figure 10c. As this is the period doubling case, we should only expect two
time scales, as shown in the IMFs. The same case will require many harmonics,
but the harmonics fail to give any indication of period doubling, because the
harmonics represent the waveform deformation instead of the period doubling.
The Hilbert spectrum of the result is presented in Figure 11a (see color figure),
in which the frequency of the first component fluctuates over a considerable
range. But nowhere is the frequency value higher than 3 Hz. The wavelet spectrum for the same case would have harmonics for very high frequency, as shown
in Huang et al (1998a). If we compute the marginal spectrum and plot them
together with the Fourier spectrum in Figure 11b, the difference is also clear:
The lack of harmonics in the representation increases the clarity of the final
result. Furthermore, the main peak of the Fourier spectrum represents only a
global weighted mean frequency. Its does not represent any true value during
the oscillation.
With these examples, we have demonstrated that the new idea of intra-wave
frequency modulation can easily depict the minute variations of the waves in
the IMF component and the data. Again, with the Hilbert spectrum as a guide,
the unevenness of the intra-wave frequency variation can be shown to have
one-to-one correspondence with the variations of the waveform in the data.
Comparison with the Hamiltonian Solution
From the above examples, one can see that Hilbert spectral analysis offers
more detailed information than the Hamiltonian system, in which the averaged
frequency is defined as
∂J
= 0,
∂t
and
ω=
∂θ
∂ H (J )
=
,
∂t
∂J
with J as the averaged action density, defined by
ZZ
1
J=
dp dq,
2π
(28)
(29)
in which θ is the angular variable and H is the total Hamiltonian in terms of
the action density variable. In these canonical expressions, the most important
parameter is the averaged period or frequency, based on which the Poincaré
section and the modern topological view of the dynamic system are built. With
such a view, the shape of the phase plane is not as important as the time needed
to trace a full cycle. As long as they are closed curves, they are topologically
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Figure 11 The Hilbert and Marginal spectra for the Rössler equation solution. The peak of the Fourier spectrum
is not any real scale of the oscillation, but a weighted mean.
NONLINEAR WAVES: THE HILBERT SPECTRUM
439
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equivalent. Yet the different shapes of the phase curves represent different details
of the oscillations. Such details can be represented only by the instantaneous
frequency, as shown above. The motion described by nonlinear equations clearly
requires the instantaneous frequency variation to specify its full physical details.
Thus, the Hilbert view is preferred over the previous view of classical nonlinear
mechanics. We will now use the new method to view nonlinear water wave
problems.
WATER WAVE PROBLEMS
Now we will turn to real physical phenomena, the problem of water waves.
All water waves are nonlinear (Whitham 1974); therefore, harmonic analysis
has always been an inseparable part of wave phenomenon studies. Yet such
an approach offers a confused view: As water waves are dispersive, waves of
different frequencies will propagate at different phase velocities. In terms of
harmonics, however, we are forced to separate the waves into two categories:
free waves and bounded waves. Harmonic components do not obey the dispersive relationship. Consequently, for a given wave component of certain
frequency and wave number, one must first determine whether it is a free or
a bounded wave before discussing its propagating properties. For a random
wave field, the simple, direct, and logical way to represent it is through its spectrum. The harmonics in the Fourier spectrum, however, create a real problem
in spectral analysis of how to determine which component is free and which
is bounded. In the traditional Fourier view, the typical spectrum has a rather
narrow peak and a wideband tail. Near the peak region, the waves are mostly
free waves, which propagate according to the dispersion relationship. Toward
the tail, the waves are mostly harmonic in nature, but even here, free waves are
still possible. Therefore, for any given frequency or wave number, the waves
can either be free or bounded harmonics of other free waves. As bounded harmonics, a particular wave can be the harmonic of the free fundamental waves
with 1/n times its frequency. Thus, the true nature of any component in a wave
spectrum can never be exactly determined. This is the consequence of using
Fourier analysis.
Thus we must point out here that the harmonics are a mathematical artifact.
The characteristics of nonlinear water waves are represented in the deformation of the wave form. Now, we will examine the nonlinear wave problem with
Hilbert spectral analysis. The central idea is to use intra-wave frequency modulation to explain wave form deformation. Using the nonlinear wave phenomena
as examples, we can contrast the different views and gain new insights, which
will also help us in interpreting more complicated cases in natural phenomena
with high degrees of freedom. We will start with the classic Stokes wave.
440
HUANG ET AL
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The Stokes Wave
The Stokes wave is one of the first successes of a mathematical description of
natural phenomena (Stokes 1847). The classical Stokes wave profile reveals the
nonlinearity by its sharpened crests and rounded-off troughs. Longuet-Higgins
(1963), Huang et al (1983, 1984, 1990a,b) and Shen et al (1994) have modeled
the asymmetric form, which gives the skewness in the water surface elevation distribution. In those attempts, harmonics were used as a mathematical
tool. As they are modeling the waveform deformation, that approach is perfectly legitimate. All the harmonics, however, can model only the up-anddown asymmetry. Front and back asymmetry is known to exist and has been
modeled by Longuet-Higgins (1982). We will see what the Hilbert view can
reveal.
A short section of the wave record used by Huang et al (1998a) is reproduced
in Figure 12. Applying the EMD to these data produced eight components.
The most important one is the second component, which accounts for almost
all the energy of the data. Its Hilbert spectrum is given in Figure 12a, while
the corresponding Morlet wavelet spectrum is given in Figure 12b, all with the
wave profile superimposed on them. Clearly, the waves are nonlinear, for the
Hilbert spectrum shows instantaneous frequency modulation, the hallmark for
nonlinear effects. The fluctuation of the frequency is not exactly symmetric
with respect to the wave profile, but exhibits a slight phase shift toward the
wave front, as shown in the detailed plot of the Hilbert spectrum. The highestfrequency part of the wave was always seen to be aligned with the wave front,
indicating that this part of the wave has a higher instantaneous frequency, or
a sharper change in its phase. The lowest-frequency part of the wave always
aligned with the wave back and the trough. This is in general agreement with
the sharpened crest and rounded-off trough profile, but the description is even
more exact: The Hilbert spectrum also pointed out the front-back asymmetry
as modeled by Longuet-Higgins (1982). In that study, Longuet-Higgins also
invoked a shifted phase for the harmonics. The front-back asymmetry can also
be seen from the corresponding wavelet spectrum shown in Figure 12b, in which
the harmonics are concentrated slightly in the front of the wave crest. Such a
detail could never have been detected with standard Fourier spectral analysis.
This also indicates that the traditional Stokes wave model does not give a true
description of the water waves.
The marginal spectra from both the Hilbert and the wavelet spectra are shown
in Figure 12c, together with the Fourier spectrum. This comparison again shows
the difference between the Hilbert and Fourier views: In the Hilbert view, there
are no harmonics, but there are many sub-harmonics. This, too, serves as an
indicator of nonlinearity. The frequencies of the waves are modeled by fluctuations in frequency from time to time in the Hilbert view, while the same change
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Figure 12 The selected Hilbert, Wavelet and their marginal spectra for the laboratory data of the Stokes
waves. Both Wavelet and Hilbert spectral analysis reveal the front-and-back-asymmetry. The Hilbert spectra
offers better frequency resolution.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
441
is modeled as superimposed constant frequency and amplitude sinusoidal components in the Fourier view. These Fourier components are a mathematically
correct decomposition for the data, but they do not make physical sense, because
pure sinusoidal waves are not a solution for any equation governing water surface motions. The wavelet spectrum, while correctly depicting the front-back
asymmetry, gives very poor frequency resolution. By comparison, the Hilbert
view gives an overall superior representation of the phenomena for both time
variations and frequency resolution. Now let us move to the wave evolution
problem.
Wave Evolution: Fusion
In nonlinear wave dynamics, there is an intriguing problem regarding wave
evolution. In numerous controlled experiments (Lake et al 1977; Lake & Yuen
1978; Melville 1982; Su et al 1982; Chereskin & Mollo-Christensen 1985; and
Huang et al 1996) the main frequency is seen to shift to a lower frequency, a
downshift. This innocent phenomenon presents a serious conflict with wave
theory.
According to the kinematics of wave trains, the movement of a constant phase
is given by
θ(x, t) = constant t
(30)
in which θ(x, t) is a slowly varying phase function of position and time. The
wave number k and frequency n can be defined as
k = ∇θ,
n=−
∂θ
.
∂t
(31)
Both the wave number and frequency are also assumed to be slowly varying
functions of time and position. From Equation (31), one can immediately obtain
the kinematic conservation equation of the waves as
∂k
+ ∇n = 0.
∂t
(32)
From Equation (32), the frequency of a stationary wave train should be constant. The laboratory setting is precisely the stationary case, yet the frequency
downshift has been observed routinely.
Theoretical study of the downshift problem has developed almost in parallel
with the experimental side. The first attempt to model the downshift was based
on the nonlinear Schrödinger (NLS) equation (Yuen & Ferguson 1978a,b). The
results produced by this approach, however, predict only cyclic recurrence of
downshift and upshift. Later, the problem was studied with the modified nonlinear Schrödinger (MNLS) equation, derived by Dysthe (1979) with the added
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HUANG ET AL
slow drift term and used by Lo & Mei (1985); the wideband case of the nonlinear Schrödinger equation derived by Trulsen & Dysthe (1996); the Zakharov
integral equation used by Caponi et al (1982); and the exact hydrodynamic
equations used by Dold & Peregrine (1986). All the studies found recurrence
in two-dimensional wave trains. Yet, by adding a simulated wave-breaking term,
Trulsen & Dysthe (1990) were able to obtain permanent downshift. By adding
wind and eddy viscosity, Hara & Mei (1991) also found downshift. With these
results, most investigators believed that the dissipation mechanism must be important. Such a conclusion was further supported by studies by Hara & Mei
(1994); Poitevin & Kharif (1991, 1992); Skandrani et al (1996); Uchiyama &
Kawahara (1994); and Kato & Oikawa (1995), all with some type of damping.
Recently, Trulsen & Dysthe (1997) extended the investigation to threedimensional cases, and found that a downshift is possible by allowing oblique
sideband perturbations. A quantitative analysis of past results showed that all
are within the possible range of three-dimensional perturbations. With one exception (Huang et al 1996), in all those studies, theoretical or experimental, the
results were obtained through Fourier analysis. The downshift was defined as the
shift of the peak frequency of the spectrum. As shown by Huang et al (1996),
the Fourier spectrum is a very poor way to analyze either the downshift phenomenon or the shift of the peak frequency of the spectrum; indeed, it is an inadequate way to quantify the downshift. Yet, Trulsen (1998) still tried to explain
the downshift (crest pairing) as a consequence of beating in linear dispersion
among different Fourier modes. Any such beating or modulation will have to be
reversible, but the downshift in water wave evolution is irreversible. There are
many unsolved difficulties in the present Fourier view of the downshift problem.
This will be illustrated through an examination of the experimental evidence.
The laboratory data were collected by Huang et al (1996) in the NASA
Air-Sea Interaction Research Facility located at Goddard Space Flight Center’s Wallops Flight Facility, Wallops Island, Virginia. The wind-wave tank is
91.5 cm wide, 122 cm high, and 1830 cm long, with an operational water depth
of 75 cm. For a complete description of the facility and its capabilities, see
Long (1992). For this example, waves were generated by a programmable wave
maker set at 2.5 Hz. Wave data were collected at eight stations along the tank
covering the fetch from 3 to 15 meters. The raw data of the wave elevations and
the corresponding Fourier spectra can be found in Huang et al (1996). They further showed that the Fourier spectra offered a very poor indicator for frequency
downshift. If we adopt the definition of the peak frequency as the measure of
frequency downshift, the only station that reported a downshift is station 8. If
one used peak frequency as a measure, then what spectral resolution should
one use? Take the data from stations 7 and 8 of the laboratory experiment as
an example. Huang et al (1996) identified the downshift based on the spectral
peak method to be between these two stations. Let us re-examine this approach
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Figure 13 Fourier spectra for two stations with different frequency resolutions, to demonstrate
that downshift of the spectral peak depends on frequency resolution.
carefully. The spectra of these two stations with various frequency resolutions
are given in Figure 13. Starting with the full data length of 6000 points, the
spectra are marked p7 and p8 in Figure 13. The spectra with 3000 points are
marked with p71 and p81; the spectra with only 1000 points are marked with
p72 and p82. The spectral pair, p7 and p8, does not show the peak downshift.
The pair p71 and p81 show a tie. Only the pair with the lowest resolution showed
downshift. Yet counting the real numbers of the waves through their total phase
angle variations has shown downshift long before the waves reach station 8,
as shown in Huang et al (1998a). The downshift started long before the peak
frequency changed. This raises a question about the definition of downshift. Is
the peak frequency change a good measure of downshift? Or is Fourier spectral
analysis a good tool for studying downshift? The answer to both these questions
is no.
Another complication arises for the spectral peak measure. Granted the peak
criterion, the downshift occurs at station 8. Yet Huang et al (1996) have counted
the waves in the laboratory data through the total phase changes. They found that
waves started to disappear at station 5. The number of waves missed increases
with the distance from the wave maker. Then what will be the state of the waves
at stations 5, 6, and 7? There should be no downshift based on spectrum peak,
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HUANG ET AL
but clearly the total number of waves has decreased. This decrease, however,
occurs only at certain very local regions. Such local change makes the data
nonstationary, the condition Fourier analysis is ill-equipped to deal with. As
shown above in the Rössler equation, the Fourier spectral peak represents only
the global mean frequency. It is not sensitive to the local change of frequency
as in the local and discrete downshift phenomena. Therefore, we conclude that
the spectral peak is not a good measure for downshift.
Huang et al (1996) opted for the use of Hilbert analysis, with which variation
of frequency can be defined much more precisely and locally. Phase variation
can be presented in two ways: first, the total phase value changes with respect
to the reference station, e.g. station 1. This revealed that the decrease of the
total phase values was an integer multiple of 2π. Secondly, the relative phase
variation can be presented in a joint distribution with the elevation. The selected
results are shown in Figure 14a–d. The discrete location of the phase variation is
Figure 14 Joint distribution of phase and amplitude and waves at different stations all relative to
the first station. Phase variation is discrete.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
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Figure 15 Fusion of two waves into one also coincides with a phase jump. Magnitude of phase
jump at 49 seconds is exactly 2π.
a sharp deviation from the traditional picture of slowly varying phase, frequency,
and amplitude. It was further shown that the wave evolution process is similar
to that of fusion, in which two waves fused into one locally and discretely at the
point where the phase jump occurred. A detailed example given in Huang et al
(1998a) is reproduced here in Figure 15, in which fusion is vividly illustrated
near the 49-second location on the time axis.
To summarize the findings on nonlinear wave evolution from the experimental study by Huang et al (1996), we have to emphasize that the wave frequency
downshift in the evolution indeed seems to be not a slowly varying process, but
rather a sudden jump. This presents a difficulty to theoretical analysis too, for
all of the theoretical models, such as NLS, MNLS, and others, are based on
the slowly varying phase, frequency, and amplitude. The process observed is
local, and the variation noted is discrete. Waves are lost in the process in which
n waves are fused into n−1 waves. This is the phenomenon of the “missing
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HUANG ET AL
crest” as observed by Lake et al (1977), “crest paring” observed by Ramamonjiarisoa & Mollo-Christensen (1979), and “fusion” observed by Huang et al
(1996). To reconcile this experimental observation with theoretical models is
a critical subject for future wave studies.
We must break with the earlier paradigm of wave analysis, and emphasize
again that Fourier analysis is not a good method for studying waves. The reasons
are many: water waves are nonlinear; therefore, we should not expect to use a
linear expansion and be able to represent it. With the Fourier expansion, the
harmonics have only a mathematical significance, but no physical meaning.
Furthermore, as the wave evolution is local, Fourier expansion simply cannot
represent this nonstationary process. As shown in the Rössler equation above,
the only way the Fourier method can represent a local frequency change is
through harmonics. But such a representation is no longer local. With these
concerns, we can examine random wave problems next.
Random Ocean Wind Waves
The logical measure of a random wave field is its various statistical measures
(Huang et al 1990a) and spectra (Huang et al 1990b). Traditionally, the spectral
representations are all Fourier based. Huang (1995) and Huang et al (1996,
1998a) proposed the Hilbert spectral analysis, which offers a new view of the
wave spectra. The data used by them were collected at a coastal tidal station at the
rate of 1 Hz. With Hilbert spectral analysis, a section of the result is presented
in Figure 15, in which the corresponding wavelet spectrum is presented in
a colored contour and the wave profile is also shown. By comparison, the
sharpness of the Hilbert spectrum is again evident; it can track minute variations
of the energy and frequency. In this comparison, the Hilbert spectrum indeed
gives a quantitative indication of energy and frequency variation with time. The
frequency variation is especially interesting, for this is the first time that any
method has revealed how fast frequency can change with time in a wave train.
When marginal spectra are computed from both the wavelet and Hilbert
spectra, the results reveal properties similar to those seen in the Fourier spectrum. Therefore, all three of the spectra are plotted in Figure 16b (see color
figure). The comparison is clear: The leakage of wavelet analysis causes such
smoothing that the result ceases to have any quantitative value. It seems that
the wavelet spectrum indeed resolves the nonstationarity to a certain degree,
but it has the poorest uniform frequency resolution.
Another interesting point is that the Hilbert spectrum contains almost no
energy beyond 0.25 Hz, while the Fourier spectrum has a power law tail to
the limit of the Nyquist limit. The form of the spectral tail has been studied
extensively (see, for example, Huang et al 1990b). In reality, energy in this highfrequency range is heavily contaminated by harmonics (Huang et al 1981). As
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Figure 16 A selected section of the Hilbert and Wavelet spectra together with the wave profile. The Hilbert
spectrum can track the frequency variation closely. The marginal spectra show that the Wavelet spectrum has very
poor frequency resolution.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
447
a result, the functional form could be a mathematical artifact. Once the true
energy content of the free wave is known, the dilemma of determining the
expected number of extrema from wave spectrum moments could be resolved
easily. As discussed above, the expected number of extrema is proportional
to the ratio of the fourth to the second moment of the spectrum. For most of
the Fourier spectra, the power law form of the spectral tail makes the fourth
moment unlimited. The Hilbert spectrum gives a practical cut-off frequency,
an elusive limit that for some time has bothered many investigators working on
statistical representations of the wave field.
Other than the cut-off limit, the experimental verification of the form of the
equilibrium range originally proposed by Phillips (1958) should now also be
re-examined in light of the new Hilbert view. As the Hilbert spectrum is truly
based on the local scale without contamination of the harmonics, it should be
used in testing the theoretical result based on the local scale dynamics. Whether
the spectral form should be slightly modified from that used in the more recent proposals by Phillips (1985); Toba (1973); Phillips (1977); Kitaigorodskii
(1983); Banner (1990); and Belcher & Vassilicos (1987) is a problem that needs
to be resolved with more studies.
In addition to the spectral form, the wave train properties can also be studied
by Hilbert transform as shown by Huang et al (1996), in which they found
a strong indication of the discrete characteristics of the wave field. Such an
observation was supported indirectly by the studies of Shen & Mei (1993). This
is another problem needing further study.
TURBULENCE DATA
Turbulent flow is both nonstationary and nonlinear. Several heuristic models
are presently competing to represent the flow. A first hypothesis assumes the
turbulence fields consist of superimposed waves; then turbulence is the result
of exchanging energy among the waves of comparable wave numbers. A second hypothesis assumes the turbulence fields consist of localized vortices that
are locally coherent. These vortices are highly nonlinear, yet they could also
maintain their identities without significant interactions among them. A third
hypothesis assumes the turbulence fields consist of superimposed wave packets
like eddies. This is the wave model with intermittence. And finally, a fourth hypothesis assumes the turbulence is characterized as pure noise. These views are
consistent with the more rigorous mechanical approach presented in Sagdeev
et al (1988), where the flow fields are divided into weak and strong turbulence.
In weak turbulence, flow can be represented by weak interactions among waves
of comparable wave numbers, while in strong turbulence, the nonlinearity of
the waves is strong even if the interactions among them are weak. To identify
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HUANG ET AL
the basic building block is an elusive goal (Pullin & Saffman 1998). In fact,
most phenomenological studies of turbulence are confined to probabilistic and
spectral properties as reviewed by Farge (1992) and Nelkin (1994).
Traditionally, most turbulence data have been analyzed by Fourier-based
methods. As pointed out by Farge (1992), a great risk of uncritical use of the
analysis is to misinterpret the functions used in the analysis as characteristic
of the phenomena. Turbulence is nonlinear and nonstationary; Farge (1992)
hence rightfully argued that a localized expansion should be preferred over the
space-filling trigonometric functions used in Fourier analysis. Consequently,
she proposed wavelet analysis as the solution (see, for example, Meneveau
1991). Farge’s objection is the same as that of Huang et al (1998a) on the
application of Fourier spectral analysis to nonlinear and nonstationary data.
Based on Huang et al (1998a) and the argument presented above, Hilbert spectral
analysis should be a better tool. Hilbert spectral analysis has already been
applied to a section of wind data measured with a Pitot tube over the water
surface during the initial stage of wind-wave generation. But the data rate is too
low to be useful in investigation of turbulence. We present some recent results
using the Hilbert spectrum approach on the universal equilibrium subrange of
turbulence.
According to Kolmogorov (1941), at infinite Reynolds number, all possible
symmetries should be restored locally, and all turbulent flows are self-similar.
At this stage, the small-scale statistics are uniquely and universally determined
by the mean energy dissipation rate, ε, and a scale, I. Then, through a dimensional argument, he postulated that the energy spectrum, E(k), at this range
should be
E(k) ∝ ε2/3 k −5/3 ,
(33)
in which k is 1/I. This is the famous −5/3 law. Numerous observations have
confirmed this formula (Frisch 1995). Yet problems still exist. On the theoretical side, this theory did not include small-scale eddy intermittence effects,
which were observed first by Batchelor & Townsend (1949). During the last 50
years different models were proposed successively, but not one of them has been
firmly proven to be even a good approximation up to now. Among these models, the first was proposed independently by Kolmogorov (1962) and Obukhov
(1962). They conjectured that the energy transfer to small scales was a selfsimilar cascade with an associated multiplicative process that was approached
by a lognormal distribution of the dissipation rate. Novikov & Stewart (1964)
proposed another multiplicative process, which is usually called the black and
white model. Mandelbrot (1974) conjectured that in the regions where this process takes place, the energy dissipations are a self-similar fractal subset, and
that outside this fractal subset there is no dissipation. This model is essentially
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Figure 17 The wind tunnel turbulence data, with the Hilbert, singularity, and marginal spectra, respectively.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
449
the same as that of Novikov & Stewart (1964). Parisi & Frisch (1985) modified Mandelbrot’s fractal subset to a multifractal subset where the dissipation
is strong in one section and weak in another section for any given scale, rather
than absolutely null. The corresponding model resulting from this is named the
multifractal model (Meneveau & Sreenivasan 1991).
On the experimental side, all confirmations to date are based on the Fourier
spectrum. As the scale is strictly local and the flow nonlinear, and because
the Fourier spectrum is more global and linear, it would certainly be more
desirable to have a more local measure of the scales to test the theory. This
desire apparently prompted Farge (1992) to propose wavelet techniques as an
alternative. Unfortunately, wavelet analysis lacks scale resolution, and is also
linear. Consequently, wavelet analysis has not produced any definite answer
despite numerous attempts. With the introduction of EMD and Hilbert spectral
analysis, we now have a method to accurately visualize the characteristic scale
at any given location. The method can also help us resolve the hierarchical
structure of smaller and larger eddies. The data shown in Figure 17a (see color
figure) were taken in the turbulent boundary layer of a hot plate in a wind
tunnel. The mean axial speed is 13 m/s with a Reynolds number of 3.12 × 106 .
Sampled at a rate of 20 kHz, the total data length is 8192 points. With the EMD
decomposition, this data set produced 11 IMF components. All the components
are of comparable magnitude, and the velocities seen are highly intermittent.
Two typical short sections of the data are plotted in detail in Figure 18a–b.
Two types of events stand out in Figure 18a: First, there are large regions
of intermittency (marked by A). Second, the intermittent region violated the
assumption of the curdling process as required in the multifractal model (marked
by B). On detailed examination, we found that events A cover over only a small
portion of the data length, but event B occurs as a rule rather than an exception.
In Figure 18(b), the cascade model seems to work well. Events A and B imply
that turbulence is most likely not a multifractal process.
With these IMFs, the Hilbert spectrum is constructed with the same frequency
resolution as the Fourier spectrum as shown in Figure 17b. The energy distributions are uniform throughout the time-frequency space, but also are intermittent.
The marginal Hilbert together with the Fourier spectra are shown in Figure 17d.
The Fourier spectrum follows a curved trend. If a −5/3 straight line is drawn,
it seems to fit only a small section of about one decade of around 1000 Hz
frequency range. The Hilbert spectrum shows a very broad, constant sloping
base covering about three decades. It then is seen to bend into a larger negative
slope around 5000 Hz, the frequency at which the viscous effect is becoming
dominant. Since the Hilbert spectral analysis does not admit harmonics, the
appearance of the marginal Hilbert spectrum represents motions of the physical
scale locally. The dominant range is similar to the inertia range proposed by
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HUANG ET AL
Figure 18 Selected sections of the intrinsic mode function expansion of the turbulence data.
Events A and B show the conflict with the fractal hypothesis.
Kolmogorov (1962). The slope of the spectrum, however, is slightly higher
than the −5/3 power. The meaning of this difference needs to be examined.
Finally, there are an increasing number of investigators (Parisi & Frisch
1985; Saddeev et al 1988; Meneveau & Sreenivasan 1991) who have proposed
to describe turbulence as a fractal process. This has prompted Aurell et al (1992)
to point out that a spurious multifractal result is a possibility. In fact, when the
data used here were processed in the same way as by Meneveau & Sreenivasan
(1991), the resulting singularity spectrum shown in Figure 17c also suggested
a multifractal conclusion. But detailed examination of the decomposed data
in Figure 18a offered some contradiction to the curdling process. Thus, the
multifractal state could indeed be spurious.
All these studies, however, are phenomenological. The results here are used
primarily to highlight the new method for data analysis. The real dynamics need
NONLINEAR WAVES: THE HILBERT SPECTRUM
451
to be studied through an approach totally different from these cited here (see
Pullin & Saffman 1998).
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DISCUSSION
Through various numerical and real data we have shown that the new Hilbert
view indeed provides a clearer picture of the underlying physical processes.
Influenced by the omnipotent perturbation methods of the past for weakly nonlinear phenomena, data analysis has been dominated by Fourier-based analysis. A few more remarks on Fourier analysis are necessary here. Although
the Fourier transform is valid under extremely general conditions (see, for example, Titchmarsh 1948), to use it as a method for physical interpretation of
frequency-energy distribution was not the original intention. The Fourier expansion was originally proposed to approximate any function to any degree
of accuracy mathematically. In such an expansion, each component certainly
serves its mathematical function in the approximation, but no more. In spectral
analysis, the Fourier spectrum has indeed provided a general method for examining the global energy-frequency distributions; however, in this application,
additional physical meanings are assigned to the components, an extension
whose physical meaning has never been clearly established. For Fourier spectral analysis to be meaningful, there are some crucial restrictions: the data
must be linear, and strictly periodic or stationary. Furthermore, to have good
resolution, the data have to be long. Few of the data sets, from either natural
phenomena or artificial sources, can satisfy all these strict conditions of stationarity. Additionally, most of the natural systems are nonlinear. Almost all the
data we face will have one or more of the following problems: the total data
span is too short; the data are nonstationary; and the data represent nonlinear
processes. Facing such data, Fourier spectral analysis is of limited use. For lack
of alternatives, however, Fourier spectral analysis is still applied. As a result,
the term spectrum has become almost synonymous with the Fourier transform
of the data. The uncritical use of Fourier spectral analysis and adoption of the
stationary and linear assumptions may give misleading results. The problems
can be illustrated by the following arguments:
First, Fourier spectral analysis transfers the data from the time to the frequency domain with constant amplitude and frequency trigonometric terms. In
the frequency domain, the relationship with time is totally lost. Thus Fourier
spectral analysis suffers an inherited defect for representing nonstationary data.
As the Fourier spectrum utilizes uniform harmonic components globally, it
therefore needs many additional harmonic components to simulate either the
nonstationary or the nonlinear variations of the data. To illustrate the above
point, let us consider a delta function that has a phase-locked white Fourier
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HUANG ET AL
spectrum. Here, many Fourier components are added to simulate the nonstationary nature of the data in the time domain, but their existence diverts energy
to a much wider frequency domain. Constrained by the energy conservation
principle, each component will have a relatively low energy content. The total
energy is uniformly distributed over the whole time domain, which is not physical for a nonstationary process. Thus, the Fourier spectral components might
make mathematical sense, but they make no physical sense.
Second, Fourier spectral analysis uses linear superposition of trigonometric
functions; therefore, it needs additional harmonic components to simulate the
deformations in wave profiles. Most of the deformations, as will be shown
later, are the direct consequence of intra-wave frequency modulations through
nonlinear effects. Thus the harmonics give a misleading energy-frequency representation for nonlinear data.
There are other variations of the Fourier-based methods, such as the spectrogram (see, for example, Oppenheim & Schafer 1989); wavelet analysis for time
series (see, for example, Chan 1995, Farge 1992, and Long et al 1993a), and
two-dimensional images (Spedding et al 1993); the Wigner-Ville distribution
(see, for example, Claasen & Mecklenbräuker 1980 and Cohen 1995); the evolutionary spectrum (see, for example, Priestley 1965); the empirical orthogonal
function expansion, also known as the principal component analysis, or singular
value decomposition method; and some miscellaneous methods such as least
square estimation of the trend, smoothing by moving averaging, and differencing to generate stationary data. All the above methods are designed to modify
the global representation of the Fourier analysis, but they all failed in one way
or the other, as discussed by Huang et al (1998a) and demonstrated here.
Finally, let us turn to the problem of nonlinearity. It has always been controversial to use the term nonlinear in association with “data”. The most convincing objection to the term nonlinear data is that all data can be decomposed
into Fourier series. Since the Fourier series is a linear decomposition, and each
component is also the solution of a linear differential equation, then it follows
that the data are the superposition of linear solutions; therefore, they should be
regarded as linear. This is the typical Fourier view. With this logic, of course,
all data are linear. There are various tests proposed by Priestley (1988), Bendat
(1990), and Tong (1990). Unfortunately, these tests give only necessary conditions. The view advanced here, to link the intra-wave frequency modulation as
an indicator for nonlinearity, also has difficulties. If one examines the classic
nonlinear system as given in Equations (22) and (27), one finds that the solution forms a nonlinear equation that has a particular characteristic, intra-wave
frequency modulation. Therefore, a nonlinear signal should have phase-locked
harmonics, while a linear signal should have only uniformly distributed phase.
Unfortunately, this condition is also only a necessary but not a sufficient one.
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NONLINEAR WAVES: THE HILBERT SPECTRUM
453
Many intra-wave frequency modulation cases could also be the solutions of
variable coefficient linear differential equations. Equation (19) is an example,
as discussed by Huang et al (1998a), and Mathieu’s equation is another. Those
variable coefficient linear differential equations can exhibit all kinds of nonlinear behavior, including the generation of chaos. A foolproof definition will
have to wait for a better understanding of nonlinear systems. For the time being,
the term is used as a means of convenience as well as an attempt to describe data
with different characteristics. Its use is very similar to that in Bendat (1990)
and Tong (1990).
CONCLUSIONS
The empirical mode decomposition (EMD) method and the associated Hilbert
spectral analysis indeed offer a powerful method for nonlinear, nonstationary
data analysis. Central to the present approach is the sifting process to produce IMFs, which enables complicated data to be reduced into amplitude- and
frequency-modulated form so that instantaneous frequencies can be defined.
These IMFs form the basis of the decomposition and are complete and practically orthogonal. The expansion in terms of the IMF basis has the appearance
of a generalized Fourier analysis with variable amplitudes and frequencies. It
is the first local and adaptive method in frequency-time analysis.
A great advantage of EMD and Hilbert spectral analysis is effective use of the
data. In EMD, we have used all the data in defining the longest-period component. Furthermore, we do not need a whole wave to define the local frequency,
for the Hilbert transform gives the best-fit local sine or cosine form to the local
data; therefore, the frequency resolution for any point is uniformly defined by
the stationary-phase method or local derivative of the phase. This advantage
is especially valuable in extracting low-frequency oscillations. Unlike wavelet
analysis, instantaneous frequency can still be localized in time even for the
longest period component without spreading energy over wide frequency and
time ranges. Still another advantage of EMD and Hilbert spectral analysis is
its application to transient data without zero or mean references; the trend or
the DC term is automatically eliminated.
Other than the practical aspect, the most important conceptual innovation
of the present study is the physical significance assigned to the instantaneous
frequency for each mode of a complicated data set. By adopting the instantaneous frequency, we can clearly define both the inter- and intra-wave frequency
modulations in a wave train. Such frequency modulations are totally lost in
Fourier spectral analysis, and only the inter-wave frequency modulation can be
vaguely depicted in wavelet analysis. Yet, both the inter-wave and the intra-wave
frequency modulations are critical in interpretation of oscillatory phenomena.
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HUANG ET AL
The former explains the wave form deformation by nonlinear effects, which
traditionally has been taken as the harmonic distortion; the latter explains the
dispersive propagation of waves. Intra-wave frequency modulation offers new
insight into nonlinear oscillation systems in more detail than the modern topological treatment. By adopting the instantaneous frequency, we have eliminated
the need of not only higher harmonics to simulate nonlinearly deformed waves,
but also spurious harmonics to simulate nonstationary data. We believe this
new method can give us new physical insight in all other nonlinear and nonstationary phenomena. Instantaneous frequency can be defined only through the
IMF, which is defined here based on local properties of the data rather than the
global restrictions proposed before.
Hilbert spectral analysis is also a tool. Its use in exploring the full physical
meanings of complicated data is only now beginning, and associated properties
of the marginal spectra need to be explored.
ACKNOWLEDGMENTS
The authors would like to thank Professors T. Y. Wu of the California Institute
of Technology and O. M. Phillips of the Johns Hopkins University for their
continuous guidance and encouragement over the years. We also would like
to thank Professor Fred Browand of the University of Southern California for
sharing the turbulent boundary data with us. NEH would like to thank Professor
Wu especially for the hospitality extended to him during his sabbatical visit at
Caltech. NEH and ZS are supported in part by grants from NSF (NSF-CMS9615897), US Navy NSWC, and NASA RTOP program (622-47-11). SRL is
supported in part by a NASA (N00014-98-F-0412) RTOP program (622-4713). NASA has filed for a patent for the algorithms of the EMD and Hilbert
spectral analysis methods.
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Annual Review of Fluid Mechanics
Volume 31, 1999
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CONTENTS
Linear and Nonlinear Models of Aniosotropic Turbulence, Claude
Cambon, Julian F. Scott
1
Transport by Coherent Barotropic Vortices, Antonello Provenzale
55
Nuclear Magnetic Resonance as a Tool to Study Flow, Eiichi Fukushima
95
Computational Fluid Dynamics of Whole-Body Aircraft, Ramesh
Agarwal
125
Liquid and Vapor Flow in Superheated Rock, Andrew W. Woods
171
The Fluid Mechanics of Natural Ventilation, P. F. Linden
201
Flow Control with Noncircular Jets, E. J. Gutmark, F. F. Grinstein
239
Magnetohydrodynamics in Materials Processing, P. A. Davidson
273
Nonlinear Gravity and Capillary-Gravity Waves, Frédéric Dias,
Christian Kharif
301
Fluid Coating on a Fiber, David Quéré
347
Preconditioning Techniques in Fluid Dynamics, E. Turkel
385
A New View of Nonlinear Water Waves: The Hilbert Spectrum, Norden
E. Huang, Zheng Shen, Steven R. Long
417
Planetary-Entry Gas Dynamics, Peter A. Gnoffo
459
VORTEX PARADIGM FOR ACCELERATED INHOMOGENEOUS
FLOWS: Visiometrics for the Rayleigh-Taylor and Richtmyer-Meshkov
Environments, Norman J. Zabusky
495
Collapse, Symmetry Breaking, and Hysteresis in Swirling Flows,
Vladimir Shtern, Fazle Hussain
537
Direct Numerical Simulation of Free-Surface and Interfacial Flow, Ruben
Scardovelli, Stéphane Zaleski
567