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1 Centre for Nonlinear Dynamics, McGill University, Montreal, Quebec, Canada H3G 1Y6; 2 Institut für Mathematik, Universität Graz, A-8010 Graz, Austria; and 3 Department of Mathematics and Computer Science, Macalester College, Saint Paul, Minnesota 55105
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ABSTRACT |
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The power spectrum of human heart rate (HR) measured
over 24 h exhibits "power-law"
1/f
-type spectral behavior with
1. We investigate possible nonstationarity in time of the exponent
using maximum likelihood estimation, which allows relatively short data
segments to be used. Examination of 24-h HR records from ambulatory
normal and congestive heart failure (CHF) subjects indicates that the
power-law structure of HR is nonstationary. In addition,
varies
with time scale and is different for normal (
1) and CHF
(
1.5) subjects. Simulations suggest that a possible mechanism
underlying the observed power-law spectrum may be a switching between
values of
near zero (white noise) and near two (Brownian motion).
This mechanism generates power-law forms quantitatively similar to CHF
subjects when the switching occurs very rapidly and similar to normal
subjects when the switching is less rapid.
power law; control; self-similarity; model; surrogate data
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INTRODUCTION |
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IT HAS BEEN NOTED by numerous investigators
(10, 12, 16, 20) that the variance of human heart rate (HR) or R-R
intervals tends to increase when examined on longer and longer time
scales. When examined using spectral analysis, this increase has the
form of a "power law" where the squared amplitude of the Fourier
transform at frequency f is proportional to
1/f
. Generically, this form is called
"one-over-f noise" and indeed it is found empirically
that in heart rate
1, as first reported by Kobayashi and Musha
(10).
Figure 1A shows a 2-h segment of a
24-h R-R interval time series. Figure 1B depicts the power
spectrum P( f ) for the entire 24-h record.
One can divide the power spectrum into two main parts. At frequencies
above ~0.02 Hz (or, equivalently, time scales <50 s) the HR does
not have 1/f structure and in fact shows the two well-known
broad peaks: one at the frequency of respiration and one at a time
scale of 10 s. At frequencies below ~0.02 Hz the power spectrum is
well approximated by a straight line of slope
1. Because the
power spectrum is being plotted on log-log axes, this straight line
corresponds to a power-law relationship P( f ) ~ 1/f
.
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Although 1/f
noise is observed in a wide
diversity of physical, technological, and biological systems, e.g.,
river flows (4), traffic densities (9), and loudness fluctuations in speech and music (22), there is currently no general explanation for
its ubiquity and no generally satisfactory framework for its modeling
in specific instances. In cardiac physiology, where there are numerous
interacting control systems and adapting mechanisms with a wide range
of time scales (3), it is of interest to know why a single exponent
should describe the relationship between fluctuations on time scales
from 1 min to several hours.
We are interested here in two questions: Is the exponent
constant,
independent of frequency (for f < 0.2 Hz)? Is the exponent
constant over time?
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METHODS |
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The fundamental method we employ for assessing possible changes in
with time involves dividing a 24-h R-R interval time series into short
segments, computing an estimate
in each segment and checking
whether
is statistically significantly different from one
segment to another. However, we confront the trade-off between bias and
variance: to track rapid changes in
we need to use short segments,
but to get reliable estimates
we want segments to be long.
Although this trade-off is unavoidable, we optimize our estimates
by using an efficient maximum likelihood estimator (MLE) of
. This MLE has been found to provide estimates that are superior to
linear regression on the logarithmic power spectrum or to
Hurst-exponent type estimators (13, 1).
Time-Rescaling Analysis
When one divides a long time series into segments, one is implicitly setting the lowest frequency that can be considered in each segment. If we wish to include frequency f in the analysis, our segments must have length at least 1/f s. For instance, for frequency scales down to 0.0002 Hz, data segments must be >5,000 s.The interval Ts between samples sets the highest
frequency that can be considered (1/2Ts). In
studying the 1/f
structure of R-R intervals, we
would like to be able explicitly to set both the upper and lower
frequency bounds. When using a fast Fourier transform (FFT) estimator
this is straightforward: explicitly set the frequency window over which
linear regression is performed and ignore other frequencies. The MLE
technique does not directly permit this, but we can still impose
frequency bounds via the segment length and by setting the sampling
interval Ts. The method that we have developed,
which we term time rescaling analysis (TRA), consists of the following
steps: 1) interpolate the raw R-R interval sequence into evenly
spaced samples with Ts = 0.5 s; 2) pick a
lower and upper frequency of interest (flower and
fupper); 3) anti-alias filter and resample
the time series with a sampling interval of Ts = 1/2 1/fupper; 4) divide the
resampled time series into segments of length (L) = 1/flower (in the work reported here, we make our
segments L = 256 points, giving
flower = fupper/128 =
fupper/27; thus we cover 7 octaves of
the frequency scale). 5) For each segment, use MLE to compute
the estimate
.
At this point, we have a time series of
: one estimate for
each segment. This time series can be examined directly to detect changes in
over time, as in Figs.
2A and 3A.
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To investigate how
depends on the frequency
flower, we repeat steps 1-5 for
several different values of flower, as seen in
Figs. 2B and 3B, where the results are formatted in
terms of Ts = 1/2Ts.
Assessing Statistical Significance
Figure 2 shows the results of applying the TRA technique to a synthetic signal whose power spectrum (estimated from the FFT) is a perfect power law with
= 1. It can be seen (Fig. 2A) that the estimates
vary somewhat from segment to segment. Because the synthetic
signal is constructed to be stationary, we know that this is sampling
variability and results from the fact that each segment is a sample
from the perfect power-law signal.
In considering whether nonstationarity in
is responsible for
segment-to-segment variation in
, we need to take into account sampling variability. One way to do this is to use synthetic data of
the sort generated in Fig. 2 that has a perfect power-law structure. This approach was used in previous work studying the sampling distribution of the MLE estimator (13). However, it has not yet been
established that R-R interval data is indeed perfect power-law data. We
have therefore used a more general technique for generating synthetic
data: the method of surrogate data (7, 8, 19).
Surrogate data are obtained in the following way: 1) take the
Fourier transform of the original time series; 2) randomize the
phases at each frequency to be uniformly distributed in [0, 2
];
3) take the inverse Fourier transform.
Because the amplitude of the Fourier transform remains unchanged in step 2, the power spectra of the surrogate data and the original data are identical. Different realizations of surrogate data, all with the same power spectrum, can be generated by using different random phases in step 2.
Surrogate data exhibit the following important characteristics. 1) By construction, surrogate data are equivalent to linear filtering of stationary Gaussian white noise. 2) The process that generates surrogate data is stationary, i.e., the coefficients of the filter process remain constant as do the properties of the Gaussian white noise.
Thus surrogate data stem from a linear and stationary process. We note
that although surrogate data have the same linear correlations as the
original data, any nonlinear correlations in the original data do not
appear in the surrogate data. Insofar as nonlinear correlations exist
in R-R interval data [a controversial issue that is the subject of
current research (6, 7, 14, 17)], the surrogate data will be
qualitatively different from the R-R interval data. However, although
nonlinearities might possibly be important in the generation of
1/f
noise, estimates of
based on spectral
analysis or the MLE method used here will be insensitive to the
nonlinear correlations in the data. Therefore we claim that surrogate
data provide an appropriate statistical technique for estimating the
sampling distribution of the MLE estimator. However, without a specific
model of how some nonlinearity underlies 1/f
noise, we do not know how to construct an empirical test of the validity of this claim.
Using surrogate data, we can estimate the sampling distribution for
for a stationary process with the same power spectrum as the
24-h R-R interval data. We use three approaches to investigating whether the distribution from surrogate data differs from that of the
original R-R interval data; we term this the stationarity-in-time analysis.
The first approach is to graphically display the histograms of the
segment-by-segment estimates
for the R-R interval data and a
surrogate data set. If the R-R interval data have a nonstationary
,
the histogram should be broader for the R-R interval data than for the
surrogate data. In addition, we plot out a time series of
versus time for both the R-R-interval data and one realization of
surrogate data.
The second approach is to quantify the width of the distribution of
using the interquartile range and compare the width of the
estimates
for the R-R interval to the estimates for 10 different realizations of surrogate data using a two-sided t-test.
A third approach is to characterize general differences in the
distribution using the Kolmogorov-Smirnov (K-S) test (15, 21). The K-S
measure d is defined as the maximum value of the absolute difference
between two cumulative distribution functions. For each R-R interval
time series we obtain a set of estimates
. Ten realizations of
surrogate data are used, producing 10 sets of
from stationary
processes. First, we compare the data estimates to each of the 10 surrogate estimates using the K-S statistic and obtain 10 measures D = (d1, d2, ... , d10). Then, we compare each of the surrogate estimates to each other and obtain 10 * 9/2 = 45 measures Ds = (ds1,
ds2, ... , ds45). Finally, we perform
Student's t-test to determine whether the two samples D and
Ds could have the same mean.
We note that surrogate data were developed originally (19) to detect
nonlinearity in possibly chaotic data. This use involves employing a
statistic that is sensitive to nonlinear structure. Here, we use a
statistic
that is based on the autocorrelation function and
hence models the signal as linear. Because of this, differences between
the surrogates and the test data do not point directly to nonlinearity
of the test data. Instead, they reflect other violations of the null
hypothesis associated with surrogate data, in particular the
stationarity of surrogate data.
Illustration of the Techniques Using Synthetic Data
To illustrate the stationarity-in-time and TRA analyses, we consider three synthetic time series: 1) a "perfect" stationary 1/f time series where
is constant in time and the same at
all frequencies; 2) a time series where
changes in time but
is the same at all frequencies at each time; 3) a time series
where
is different for different frequency bands, but is constant
in time.
Stationary in time, independent of frequency.
A perfect 1/f time series of length 65,536 sample points was
generated using a spectral synthesis method, and then a subsample of
length 8,192 was used as our test data as in Ref. 13. A length of 8,192 is roughly the same as the 24-h R-R interval time series when sampled
every 10 s.
are
essentially identical; the interquartile range (IQR) of the
distribution of
from the 1/f time series (IQRd) and the IQR of the distribution of
from
surrogates (IQRs) are roughly the same. The K-S
computations similarly show that the distribution of
for the
1/f time series is not significantly different than that of the
surrogates, which is underlined by a significance level P < 0.40. Thus there is no indication of nonstationarity in time here, as
would be expected for this type of synthetic signal.
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is plotted for each sampling
time Ts for each segment. For fast sampling times
(e.g., 10 s) there are many segments in the whole time series and
consequently many estimates
(plotted as x). For slow
sampling times (e.g., 100 s), there are fewer segments and thus fewer
estimates for
. Note that at a sampling time of 100 s, the
time scales comprehended by one estimation range up to 7.1 h.
There is no evidence for a time-scale dependence of
, as expected
for this type of signal.
Changes in time, independent of frequency.
The ability of MLE to track nonstationarity was tested by estimating
the exponent
of test data simulating time-varying behavior of
exponent
. The data set was generated by concatenating time series,
256 data points long, with time-varying
in the range 0.5-1.8.
As seen in Fig. 3A, the estimates
(solid line) track closely the
used in the simulation (dashed line). The surrogates show no such pattern. The histogram of
is much broader for the nonstationary data than for the surrogate data (which has more or
less the same width as in the stationary case illustrated in Fig. 2).
versus sampling
time Ts. Here
is approximately constant
over a wide range of time scales, although there is no single
in
this data set. This suggests that a nonperfect power-law process may
appear to have a
that is independent of frequency. But note
that the range of
in Fig. 3B is much wider than in
Fig. 2B, reflecting the nonstationarity of the signal in Fig.
3. This is also underlined by the results from the statistical analysis
given in Table 1, P < 0.0001.
Stationary in time, but changes with frequency.
The ability of TRA to discern variations in
at different
frequencies is illustrated by application to a time series with frequency-varying exponent
. A time series of length 216 = 65,536 was synthesized. The power spectrum (Fig.
4A) shows that
= 2 for
f < 0.0017 and
= 0.8 for f
0.0017. For the analysis, a segment of length 8,192 was extracted. The power spectrum of this segment (Fig. 4B) closely mimicks power spectra seen
in studies of HR.
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with time scale.
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as a function of frequency f than does TRA
(Fig. 5B). However, this is misleading. Only those data in Fig. 4B were used in the TRA analysis, and realistic data of
any length will always have the sampling fluctuations seen in Fig. 4B. The precise straight-line form in Fig. 4A does not
incorporate the sampling variability that must be present in any
experimentally collected data set. We encourage the reader to perform
the following experiment. Without reference to Fig. 4A, locate
the frequency at which the bend in Fig. 4B occurs. Compare your
estimate to the frequency clearly indicated in 4A. We find that
an error by a factor of two is typical.
Quantitative estimate of
from the power spectrum requires that
linear regression be performed. Figure 6
shows the result of such a regression on the power spectrum in Fig.
4B. Linear regression was performed over a window from
flower to fupper, and
was estimated as the slope of the line as a function of fupper. To facilitate comparison with TRA, we have
formatted the results as a function of Ts = 1/fupper. Figure 6 shows regressions done with
frequency windows of seven (same as used in TRA), six, and five
octaves. The shorter windows do not make clearer the sharp transition
from
= 2 to
= 0.8.
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ANALYSIS OF HEART RATE |
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We applied the stationarity-in-time and TRA analysis to 20 recordings of R-R intervals over 24 h from which abnormal beats had been deleted. These time series were provided to us by C. K. Peng and A. L. Goldberger (see Ref. 12). There were 9 healthy subjects and 11 congestive heart failure (CHF) patients.
Figures 7 and 8
show the stationarity-in-time and TRA analysis for a representative
normal subject and a representative CHF patient. In both cases,
nonstationarity in
is suggested by the broad histograms of
for the R-R interval data compared with the surrogate data.
The CHF patient shows clear sustained deviations in
from the
mean value that last for several hours.
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The TRA analysis shows that for the CHF subject
increases
from
1 at Ts near 20 s to
1.5 at
Ts near 100 s. This pattern is sustained in almost
all of the records. Figure 9 shows the TRA
analysis for all 20 records. The CHF patients typically show a higher
than the normal patients at large time scales (corresponding to low frequencies).
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The stationarity-in-time analysis is presented for all of the subjects
in Fig. 10 and Table
2. In almost all subjects, the IQR of the
distribution of
is roughly twice as large in the R-R interval
data compared with the width expected purely due to sampling
variability (as indicated by surrogate data). The K-S computations
similarly show that the distribution of
for the R-R-interval
data is different than that of the surrogates and point to this
difference being statistically significant at a level P < 0.01 in all except CHF subject 9,778.
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DISCUSSION |
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R-R interval time series show in almost all cases "mixed" process
behavior, i.e., exponent
exhibits time and frequency dependence. Similar results were also found by Meesmann et al. (11), who showed
that in the HR of young healthy subjects, periods of 1/f noise
had intermittent subperiods of white noise during the night. Ichimaru
and Katayama (5) suggest that the exponent
may be different for
each sleep stage. Di Rienzo et al. (2) found that
measured
via power-spectral regression varied with frequency f.
One possibility suggested by Fig. 3 is that nonstationarity and the
observed 1/f
pattern in HR are related. In that
figure,
1 at large Ts, although
is not constant. For instance, at Ts = 140 s,
estimates are being made using segments that span 10 h, during which
time
is varying substantially, yet
at these long segment
lengths does not vary much from segment to segment.
Although there is no general theoretical explanation for systems with
= 1, there are simple theoretical models for
= 0 (white noise)
and
= 2 (Brownian motion, the cumulative sum of white noise). Is it
possible that a system that switches between white noise and Brownian
motion might produce
= 1?
From our stationarity-in-time analysis of R-R interval data, there is
no reason to suspect that the periods of white noise or Brownian motion
might last for as long as one analysis segment (2,560 s). If this were
the case, we would expect to see values of
near 0 or 2, but
we do not. Instead, we hypothesize that the switching might occur much
faster, over say one-quarter or one-half of the analysis segment (320 s
or 640 s).
In terms of control systems, Brownian motion corresponds to control being turned off, whereas white noise variability indicates that control is on: the system may be knocked off its set point by an outside disturbance, but quickly returns to it, only to be knocked off again. But why should HR control be turned off?
HR is one of several effector variables involved in regulating the cardiovascular system. By "effector variable" we mean a feature of the system that is used to bring a regulated quantity to the appropriate level or range of levels. Other effector variables are peripheral resistence, blood volume, and vascular compliance. Examples of regulated quantities are blood pressure and blood gas levels that are directly sensed or cardiac output measured indirectly via blood gas levels and blood pressure. Note that HR is generally considered not to be a regulated quantity; it is a means to an end rather than an end in itself. Although there are baroreceptors and chemoreceptors to measure blood pressure and blood gas levels, there is no analogous receptor for HR. This suggests that HR might be allowed to drift (Brownian motion). However, drifts in HR might be punctuated by periods of resetting when control systems attempt to use HR as an effector variable and therefore HR is locked in to the appropriate value for the quantity that is being regulated.
In addition, control systems acting on very long time scales (e.g., the renal blood-volume control system) might indirectly affect HR via other feedback loops. This could cause slow, long-term drifts in HR. All told, HR might be seen as episodes of Brownian motion interrupted by episodes of white noise for short time scales, all on a background of slow trends.
To model this hypothesized structure for HR, we concatenated short
segments of Gaussian white noise and Brownian motion. For each segment,
we made a random choice between white noise and Brownian motion. As a
background, we added to each segment a linear trend with a random
direction for each segment. These trends were matched at their
endpoints. Note that none of these three processes individually produce
1/f noise: white noise has
= 0, Brownian motion has
= 2, and the piecewise linear trends have
= 2 for low
frequencies and
= 0 for high frequencies.
Figure 11 shows the histograms of the
estimated exponents
(sampling time
Ts = 10 s) for data produced by our model process where model segments 256 (Fig. 11A) and 32 data points long
were concatenated (Fig. 11B). For a model segment length of
256 data points, the estimates
are able to resolve the time
series into 1/f0 and 1/f2
segments, expressed by two main peaks at
= 0 and
= 2 in the histogram. For model segments of length 32,
is not able to resolve the time-varying character of exponent
. The histograms of
from surrogate data are substantially narrower than for the
model data, providing the same kind of evidence for nonstationarity seen in the R-R interval data.
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Figure 12A, which depicts the TRA
analysis of
vs. Ts shows a pattern
similar to that seen in the R-R interval data. We point out the
similarity of the short model segment (32 points) TRA to that found in
normal subjects, and the long model segment (256 points) TRA to that
found in CHF patients.
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Figure 12B shows the effect of deleting the local linear trends part of the model. For the short model segment ("healthy") data, there is a loss of verisimilitude.
Visual comparision (Fig. 13) of a
randomly selected segment of R-R interval data from a normal subject
and a synthetic signal from the nonstationary segments-with-trend model
of
suggests that this simple model produces realistic time series
with realistic power spectra.
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This simple model of the 1/f
structure of HR
suggests that the power-law structure of HR may be nonstationary over
fairly short intervals, similar to the 5-min segments commonly used in short-term HR variability analysis (18). It also points to a possible
difference between cardiovascular control in normal and CHF subjects.
In addition, the stationarity-in-time analysis raises the question of
whether it is possible to obtain more information about the
1/f
behavior of HR data by analyzing longer time
series. The answer might be no. The range of exponents encountered
indicates that the observed 1/f
pattern might be
a property of the interaction of the estimators with nonstationarity in
the exponent
, as we have seen in the simulations.
Perspectives
Our statistical analysis of 24-h HR records indicates that the 1/f
structure in HR fluctuates in time and that
varies with time scale. Analysis of 24-h records as a whole shows
is ~1, but analysis of short segments (~1 h) shows that
fluctuates significantly. When looked at another way, concatenating
many 1-h segments with widely varying
produces a 24-h signal with
1.
We speculatively carry this process to an extreme: using computer
simulations we show that by concatenating very short segments with
= 0 or
= 2 one produces 1-h segments where
is close to 1 but
varies significantly on either side of it and 24-h patterns with
quite close to 1. We cannot confirm this rapid-switching model by
direct measurement of
on very short segments: the statistical methods have too high a variance on the short segments and we would
need to use even shorter segments to find out when the hypothetical switching occurs.
It may be possible to assess the rapid-switching model by measurements
other than
. For instance, the amplitudes of the well-known 10-s and
respiratory HR spectral peaks may vary as cardiac control switches from
an
= 0 to an
= 2 pattern. At this point in the research, we see
the value of the model as a way of supporting and organizing the
hypothesis that the 24-h 1/f structure may be an epiphenomenon
and is the statistical result of a conceptually much different process.
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ACKNOWLEDGEMENTS |
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We thank C. K. Peng and A. Goldberger for providing us with the CHF and normal HR data used in this paper.
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FOOTNOTES |
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This study was partially supported by a "Kurt-Gödel-Fellowship" of the Austrian Ministry for Science and Research, by a fellowship from the Österreichische Forschungsgesellschaft, and by grants from the Natural Sciences and Engineering Research Council of Canada, the Fonds de la recherche en santé du Québec, and the Fonds pour la formation de chercheurs et l'aide à la recherche.
The costs of publication of this article were defrayed in part by the payment of page charges. The article must therefore be hereby marked "advertisement" in accordance with 18 U.S.C. §1734 solely to indicate this fact.
Address for reprint requests: D. T. Kaplan, Dept. of Mathematics and Computer Science, Macalester College, 1600 Grand Ave., St. Paul, MN 55105.
Received 8 April 1998; accepted in final form 14 September 1998.
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