Many methods exist for quantifying the fractal characteristics of a structure via a fractal dimension. As a traditional example, a fractal dimension of a spatial fractal structure may be quantified via a box-counting fractal analysis that probes a manner in which the structure fills space. However, such spatial analyses generally are not well-suited for the analysis of so-called “time-series” fractals, which may exhibit exact or statistical self-affinity but which inherently lack well-defined spatial characteristics. In this chapter, we introduce and investigate a variety of fractal analysis techniques directed to time-series structures. We investigate the fidelity of such techniques by applying each technique to sets of computer-generated time-series data sets with well-defined fractal characteristics. Additionally, we investigate the inherent challenges in quantifying fractal characteristics (and indeed of verifying the presence of such fractal characteristics) in time-series traces modeled to resemble physical data sets.
- spatial fractal
- time-series fractal
- fractal analysis
- fractal dimension
- topological dimension
- embedding dimension
- similarity dimension
- box-counting dimension
- covering dimension
- variational box-counting
- Hurst exponent
- variance method
- Dubuc variation method
- adaptive fractal analysis
- power-law noise
- Brownian motion
- fractional Brownian motion
In this chapter, we explore a species of fractals known as “time-series” fractals. Such structures generally may be conceived (and visualized) as functions of independent variables whose plots exhibit shapes and patterns that are evocative of the more familiar spatial fractals. However, lacking well-defined spatial characteristics, time-series fractals call for analytical tools that depart from those of the world of spatial fractals. To lay the foundation for a discussion of such analytical tools, we begin with an overview of fractal structures and traditional fractal analysis techniques. We then introduce time-series fractals and investigate the unique analytical tools necessitated by such structures. Finally, we investigate the relative fidelity of these analytical tools, as well as the shortcomings inherent in performing fractal analysis on time-series fractals of limited length and/or fine-scale detail.
2. Motivating the fractal dimension
Mathematician Benoit B. Mandelbrot often is credited with introducing the notion of a fractional, or fractal, dimension in his 1967 paper, “How long is the coast of Britain?” . In fact, however, the curious nature of coastline measurements had been discussed by Lewis Fry Richardson 6 years prior in the
Recognizing Richardson’s prior investigations, Mandelbrot notes that Richardson had indeed produced an empirical relation between a measured coast length and the smallest unit of measurement : , where is a positive constant and —but observes that “unfortunately it attracted no attention” . In Ref. , building upon Richardson’s observations, Mandelbrot introduces the formalism of a fractional, or fractal1, dimension to quantify the nature of such shapes.
Following Mandelbrot’s example, to generalize the concept of a geometrical dimension, we may begin by examining the scaling behavior of such trivially self-similar objects as a line, a square, and a cube. For example, consider a line segment of length , which can be separated into non-overlapping subsets of length , each of which is identical to the whole segment but for a scaling factor . Analogously, a square with side length may be decomposed into facsimiles of side length , each of which is scaled down from the original by a factor , and a cube of side length can be decomposed into facsimiles of side length with corresponding scaling ratio ; see Figure 1. To generalize this pattern, we may observe that the scaling ratio follows the relationship . In this relationship, is known as the
Applying the concept of a similarity dimension to less trivial shapes is straightforward in the case of exactly self-similar structures, such as structures that are constructed via iteration of a generating pattern. As an example, consider the Koch curve, illustrated in Figure 2. The Koch curve is constructed as follows: Beginning with a line segment of unity length, replace the middle third of the segment with an equilateral triangle whose base has a length of 1/3 and overlies the original line segment, then remove this overlapping base segment. The resulting figure thus consists of four line segments, each of which has a length of 1/3. Iterating this process for each new line segment yields a sequence of figures that exhibit increasingly fine structure, with the limiting state of this series exhibiting exact self-similarity, in the sense that a nontrivial subset of the shape is exactly identical to the whole. This exact self-similarity is illustrated in Figure 2, which shows that the full Koch curve may be described as being formed from four exact copies of itself, each scaled down by a factor of 1/3. Thus, we can apply the above relation to find that the Koch curve has a similarity dimension of .
The similarity dimension described above represents but one example of a plurality of dimensions that can be defined and calculated for a given figure. Indeed, the utility of the similarity dimension is limited by the fact that it applies only to figures that exhibit exact self-similarity; by contrast, the complexity witnessed in natural systems such as coastlines generally exhibits self-similarity only in the statistical sense. As an example, Figure 3 illustrates a structure that exhibits statistical self-similarity. Specifically, Figure 3 illustrates an example of a modified Koch curve formed by randomizing the orientations of the line segments as the structure is generated.
As a tool for quantifying the nature of such fractal structures that do not exhibit exact self-similarity, we now turn to the (roughly self-explanatory) “box-counting dimension,” also known as the “covering dimension.” Given a structure that extends in two dimensions2, the box-counting dimension may be determined as follows: First, superimpose a square grid with individual boxes of size over the figure in question, and count the number of boxes within which some portion of the figure in question is present (see Figure 4). Next, repeat this procedure while varying the box size and construct a plot of ; for a self-similar structure, the data should follow a linear trend with a gradient equal to the box-counting dimension
The box-counting method also may be described in more geometrically intuitive terms. For example, and as shown in Figure 4, one may observe that the set of all occupied boxes at a given length scale collectively serves as an approximation of the total structure as “observed” at the length scale . Stated differently, the set of boxes that overlap some portion of the base structure may be seen as representing a snapshot of the base structure as viewed at a resolution corresponding to the length . In general, however, the set of boxes covering the base structure cannot be expected to represent the geometric details of the structure at any length scale. For example, as shown in Figure 4, is evident that the incompatibility of the straight edges of the square boxes and the jagged boundary of the Koch curve leads to a markedly crude representation of the structure at all length scales, as each occupied box will always contain details that cannot be fully represented by that box.
While the box-counting method of estimating fractal dimension is conceptually straightforward, some care must be taken to preserve the utility of the method. For example, one must select an appropriate range of box sizes over which to examine the scaling trend, given that any observed fractal scaling trend will not persist over all possible length scales. That is, for any finite structure, it is possible to encompass the structure in a box of size , for an appropriate value of . In such a case, applying the box-counting method with boxes of size will always return a value —only one box can be filled when the box size contains the entire structure—thus resulting in an apparent fractal dimension of zero. As another example, when considering a range of box sizes , nearly all such boxes will be counted as filled, and the box count will scale as the square of the inverse box size . In this case, the box-counting method will return an apparent fractal dimension of , and we may say that the pattern “looks two-dimensional” when examined at this coarse scale. When dealing with patterns found in nature, the opposite extreme of possible length scales merits consideration as well. For a mathematically-generated fractal figure, such as a figure that exhibits structure at arbitrarily fine length scales, the box-counting method may be applied with arbitrarily small box sizes . However, naturally occurring fractal structures invariably exhibit a smallest length scale to which a scaling trend may extend. For example, while the scaling trend certainly must cease at the molecular and atomic scales, such fractal scaling behavior generally diverges at length scales many times larger than this. In such cases, applying the box-counting method at length scales smaller than a smallest feature size observed in the structure yields a number of filled boxes that scales linearly with the inverse box size ; thus, the figure “looks one-dimensional” to the box-counting analysis at these scales.
Such conditions necessitate careful determination of the appropriate range of length scales over which to assess fractal scaling behavior. This determination may be made empirically, such as by observing the range of length scales over which the scaling plot is sufficiently linear. Alternatively, this determination may be made by convention, such as may be based on statistical arguments. In practice, it is generally not known
As a further consideration in optimizing the performance of the box-counting method, one must select the position and orientation of the box grid relative to the structure in question. To the extent that the box-counting method seeks to probe an inherent quality of a structure, the observed fractal dimension should not be affected by a spatial translation or rotation of the grid with respect to the structure, since the structure itself has no preferred orientation. However, consider the case shown in Figure 5, in which the box-counting method is applied to a fractal profile. In the box-counting scheme discussed above, all boxes that contain any portion of the structure under examination are counted toward the total; applying this to the structure of Figure 5, we find that 35 boxes are filled using this box size . Suppose, however, that one is able to reposition the boxes semi-independently of one another, by translating a set of adjacent boxes within each column of width . Doing so, we find that a careful repositioning of the boxes within these columns results in the box count dropping to 29. This apparent inconsistency serves to motivate a refinement of the box-counting analysis as described above. Specifically, the “variational box-counting method” includes shifting the boxes in columns as described above so as to minimize the number of boxes needed to entirely cover the figure in question. The variational box-counting method thus serves to eliminate some of the apparent ambiguity of the traditional box-counting method. Of course, some ambiguity still remains in this amended method, given that the rotational orientation of the columns relative to the examined structure remains arbitrary. To eliminate this residual ambiguity, one may repeat the above-described variational method at a variety of rotational orientations of the grid with respect to the figure and choose the angle that minimizes for each value of . However, in practical applications, incorporating this additional variation does not significantly affect the measured dimensions.
3. Time-series fractal structures
The fractal structures discussed above generally represent examples of spatial fractal structures—that is, structures with spatial extent and whose fractal characteristics are embodied in their spatial form. However, many observable structures and phenomena exhibit fractal behavior while lacking spatial form. Another important class of structures to which fractal analysis may be directed is that of “time-series” structures—that is, structures that may be represented as a single-valued function of a single independent variable. As suggested by their name, a time-series structure may refer to some variable quantity—say, stock market prices, or atmospheric pressure—that fluctuates in time, but for the purposes of this work we intend for the term to refer to any data set or plot consisting of a dependent variable that may be represented as a single-valued function of an independent variable.
As with the spatial structures considered above, a time-series structure may exhibit fractal scaling properties in either a statistical or an exact sense, which may be quantified using the formalism of fractal dimensions. Unfortunately, the box-counting methods described above for measuring a fractal dimension are ill-suited to time-series structures. Simply put, this limitation arises from the fact that box-counting methods assess the fractal dimension of shapes that extend in space, while the spatial “shape” of a time-series structure is inherently undefined. That is, since the two axes of a plot representing a time-series data set generally represent variables with distinct units, the geometric aspect ratio of such a plot is fundamentally undefined.
As an example, consider the data set displayed in Figure 6, which plots the daily closing price of a certain technology stock over a period of roughly 16 years. Specifically, Figure 6 illustrates three representations of the same data set, with the respective
The difficulty here lies in the fact that a box-counting fractal analysis necessarily treats a figure as a spatial entity whose orthogonal dimensions have the same units. By contrast, a time-series trace such as the one displayed in Figure 6 lacks this property, but may still exhibit fractal characteristics in the form of either statistical or exact self-affinity. As discussed above, exact and statistical self-similarity describe structures whose precise details or statistical properties (respectively) are repeated as its orthogonal dimensions are rescaled by a similar factor. By contrast, exact and statistical self-affinity refer to structures whose precise details or statistical properties (respectively) are repeated as its two orthogonal dimensions are resized by independent quantities .
Due to the incommensurability of the orthogonal axes defining a time-series trace, such structures cannot exhibit self-similarity, only self-affinity. As an example, Figure 7 displays the data set shown in Figure 6 alongside a subset of the data set. When this subset is appropriately rescaled in each of the
It also is possible, albeit less common, for a time-series trace to exhibit
4. Fractal analysis of time-series traces: beyond box-counting
As discussed above, when applying a box-counting method to a time-series structure, the measured scaling properties of the structure will depend on the aspect ratio with which the data are presented, which is in turn an arbitrary choice. Accordingly, applying a box-counting method to a time-series trace will return a fractal dimension that is essentially arbitrary. Thus, it is necessary to develop fractal analysis techniques that are insensitive to such artificial geometric parameters. In the following, we survey a sampling of such techniques proposed in the literature.
Returning to the example of Figure 5, above, this figure in fact illustrates the variational box-counting method as applied to fractal profile in the form of a time-series fractal. Indeed, fractal analyses of such time-series fractal structures have traditionally been performed using the variational box-counting method [6, 7], which does offer performance improvements over the traditional fixed-grid box-counting method. Nonetheless, the variational box-counting method still suffers from a fatal flaw. To see why this is so, consider the plots shown in Figure 9.
Figure 9 illustrates the stock price data of Figures 6 and 7 represented in two plots with the price axes respectively scaled by two different factors, as well as a visualization of a variational box-count method applied at a “length” scale trading days. When the prices shown range from 0–100 USD (top of Figure 9), we find that a minimum of 37 boxes are needed to entirely cover the trace. However, when the price range is expanded to 0–1000 USD (effectively increasing the domain: range aspect ratio of the data; bottom of Figure 9), the number of boxes needed to cover the trace falls to 20. Indeed, the number of boxes needed to cover the “compressed” plot will be proportional to for all values of such that the boxes are “taller” than the range of values found within any of its columns. That is, as long as each box is “taller” than the vertical extent of the trace within each column, the trace will “look” one-dimensional.
Of course, the fundamental issue is that the concept of an “box” on a time-series trace is meaningless, since the enclosed “area” has units of (in this case) days times dollars. While it is entirely reasonable to overlay a spatial figure with boxes of a well-defined area in the case of a box-counting analysis of a spatial fractal, the concept of a square drawn on a plot with incompatible and independently scalable axes is ill-defined. In some cases, this inadequacy is resolved by adopting conventions that eliminate such ambiguity. For example, a time-series trace may be normalized in its
Developing a fractal analysis technique that is appropriate for time-series structures generally amounts to taking one of two approaches: (1) to treat the time-series structure as a geometric figure without a well-defined aspect ratio, or (2) to treat the time-series structure as an ordered record of a process that exhibits a quantifiable degree of randomness. Following the latter approach, Harold Edwin Hurst introduced a formalism for quantifying the nature of self-affine time-series structures in a 1951 paper on the long-term storage capacity of water reservoirs .
In Ref. , Hurst introduces the concept of the “Hurst exponent” , which may be understood as quantifying the character of the randomness exhibited in a time-series structure via an autocorrelation measurement. Specifically, a Hurst exponent of describes a process that is purely random, such that the value of the trace at time is entirely independent of the value at time , . By contrast, Hurst exponents in the range represent traces exhibiting positive autocorrelations, while Hurst exponents in the range represent traces exhibiting negative autocorrelations. Intuitively speaking, a positive autocorrelation may be understood as representing a trace in which a “high” value (say, relative to the mean) is more likely than not to be followed by additional “high” values, while a negative autocorrelation may be understood as representing a trace in which “high” and “low” values alternate at short time scales; see Figure 10.
The Hurst exponent of a data set may be calculated by examining the scaling properties of a “rescaled range” of the data, as follows. Consider a data set , and let represent any sequence of points within the data set. The rescaled range (
is the sample mean and
is the sample standard deviation. The quantity
is then proportional to , such that the gradient of a plot of is equal to the Hurst exponent
The Hurst exponent also may be described as a measure of long-range correlations within a data set, such that measuring these correlations as a function of interval width may provide another measurement of the Hurst exponent. As an example of such an analysis, the “variance method”3 calculates the scaling properties of the trace’s autocorrelation as a function of time interval4 via calculation of the quantity
for a range of values of . This quantity is then related to the Hurst exponent as such that a plot of is expected to be linear (within an appropriate range of values of ) with slope. 2
As another means of quantifying the fractal properties of time-series traces, we now turn our attention to a method proposed by Benoit Dubuc in a 1989 paper  on the fractal dimension of profiles. Dubuc’s proposed “variation method”5 is conceptually similar to the variational box-counting method described above, but improves upon this method by resolving the fundamental arbitrariness of drawings boxes on a time-series trace. In short, Dubuc’s variation method probes the “space-filling” characteristics of a time-series trace through measurement of the scaling behavior of the amplitude of the trace within an neighborhood as is varied.
In practical terms, Dubuc’s variation method may be implemented is as follows: Consider a time-series data set . For a given value of , define the functions and as follows:
That is, for a given value of and for each point in the trace, examine the set of points within data points of , and let and be (respectively) the maximum and minimum values of found in this range. Thus, and may be understood as traces that represent (respectively) the upper and lower envelopes of oscillation of a trace at a particular scale set by . At large values of , the traces and will be slowly varying relative to the variation present in the original data set; reducing the value of will produce traces and that each resemble the original data set with increasing fidelity (see Figure 11).
Having constructed the traces and , we then define and calculate
Conceptually, may be regarded as representing the (crucially, not necessarily integer) number of “boxes” whose total “area” would be equal to that of the envelope bounded by and . Of course, the concept of “area” is ill-defined in this context, but this is of no concern, given that we have not implied a geometrical relationship between the
As a final means of quantifying the fractal properties of time-series traces, we consider a technique known as “adaptive fractal analysis” (AFA) . Similar to Dubuc’s variation method, AFA may be broadly described as investigating the geometrical properties of a time-series trace (in contrast to the aforementioned analyses that are best understood as probing numerical correlations). For example, and as discussed above, Dubuc’s variation method may be described as quantifying the generalized “area” needed to cover a time-series trace as analyzed at different characteristic time scales; in the case of AFA, approximations to the time-series trace are generated at varying resolutions, and the fidelity of such approximations is recorded as the resolution is varied. The AFA algorithm may be executed as follows: Again, consider a time-series data set . Next, choose a window with a width equal to an odd integer , and partition the data set into overlapping subsets of length
, where and . Conceptually, each value may be thought of as representing the weighted average of the values of the two best-fit lines with values at that index, weighted so as to be inversely proportional to the distance between that index and the midpoint of the window. Repeating this procedure across all windows produces a trace that is continuous and differentiable, and that may be understood as representing an approximation to the trace at a length scale, or “resolution,” defined by
such that a plot of will be linear (over an appropriate range) with slope
5. Evaluating fractal analysis techniques
Each of the fractal analysis techniques discussed above is best understood as providing an
A noise trace, as an example of a time-series structure, may be described as a single-valued function of a single independent variable. A variety of methods exist for quantifying the statistical properties of noise traces. For example, in addition to the aforementioned measurements of space-filling characteristics and long-range correlations, a spectral analysis of a noise trace may offer a natural quantification of the trace’s statistical properties.
Power-law noise represents a significant and broad class of noise traces. Specifically, a power-law noise trace has a power spectral density given by . A noise trace characterized by thus represents noise whose spectral power density is a constant across all frequencies, while corresponds to the “noise” that characterizes many natural systems, and is known as “brown noise.” In principle, can assume any value; however, we begin our investigation by considering the case.
A “brown noise” trace characterized by is so termed owing to its relation to Brownian motion, which describes the net motion of a particle whose individual steps are random and independent. Brownian motion generally may refer to a process extending in any number of dimensions; however, we restrict our attention to brown noises that may be understood as a time-dependent plot of the position of a particle undergoing Brownian motion along one dimension. (As used herein, “Brownian motion” and “brown noise” will be used interchangeably to describe a Brownian motion in one dimension.) Given that a Brownian motion may be described as the cumulative sum of a series of random, independent steps, it is straightforward to generate a Brownian motion trace as a cumulative integral of a white noise trace. For our purposes, we define a white noise trace as a series of values with zero mean taken from a normal distribution (i.e., a Gaussian noise trace; see Figure 13). As a result, a brown noise trace is characterized by a Hurst exponent of .
Relaxing the restriction that the Gaussian noise trace consists of statistically independent increments permits consecutive increments to be positively or negatively correlated, such that the plot formed by the cumulative sum of the noise trace may be characterized by a Hurst exponent that deviates from . Such a trace is termed a “fractional Brownian motion” (fBm). Mandelbrot and Van Ness  provide a formalism for quantifying the properties of such structures as follows: Consider a conventional Brownian motion trace , where denotes time and represents the particular realization of the random function that generated the specific Brownian motion. The data set is thus a function whose increments have a mean of zero and a variance of , and whose non-overlapping increments and are statistically independent. A “reduced fractional Brownian motion” , then, is further characterized by the parameter , , and satisfies
A fractional Brownian motion trace is thus self-affine in the sense that
denotes that the two random functions and have identical finite joint distribution functions . Thus, on average, when an interval on an fBm trace is expanded by a factor of , the difference of the values at the endpoints of the interval increases by a factor of . This property represents an example of statistical self-affinity, in which the observed statistical properties within the intervals are preserved when the and axes are scaled by distinct factors (specifically, and , respectively).
Quantifying self-affinity using the formalism of the Hurst exponent motivates drawing a parallel between the Hurst exponent and the fractal dimension, as follows. Following the argument of Ref. , consider an fBm trace that extends over a total time span and a total vertical range . Dividing the time span into
The relationship is appealing in its simplicity, and indeed is frequently found in the literature; however, Ref.  is quick to acknowledge the inherent difficulty in assigning a fractal dimension to a self-affine structure, given that such a construction is predicated upon assigning an arbitrary rescaling relationship between incompatible coordinates. Mandelbrot, too, notes the apparent relation  and clarifies that this relation holds in the fine-scale limit. This disparity serves to highlight a general distinction between the Hurst exponent and the fractal dimension as descriptors of a time-series trace. Specifically, the Hurst exponent may be understood as a descriptor of
6. Relationship between fractal dimension and spectral exponent
We may continue this exercise of comparing our various statistical parameters by considering the spectral exponent as a means of quantifying the nature of a fractal trace. In practice, it is impractical to utilize a spectral analysis to evaluate the fractal properties of a time-series structure, due to the imprecision (relative to the aforementioned fractal analysis techniques) of applying a power law best-fit curve to characterize a spectral decomposition of a trace. Nevertheless, we may investigate the relationship that exists between the spectral exponent , the fractal dimension , and the Hurst exponent , so long as we recognize the imprecisions of these comparisons. In particular, the spectral exponent typically is said to relate to the Hurst exponent as , implying the relationship . This relationship may be derived by observing that the two-point autocorrelation function
for a trace is related to the quantity as
comparing this result to the aforementioned relationship
leads to the expression . However, systematic study  demonstrates that such a relationship is generally not very robust. Indeed, it is straightforward to test this robustness: In analogy to the investigation performed in Ref. , we investigated the relationship between spectral exponent and fractal dimension by generating a set of 20 noise traces, each with a length of 16,384 points and with a value between 0 and 2. Applying each of the previously discussed time-series fractal analysis techniques to each of these traces produced a corresponding set of fractal dimensions (for the variational box-counting analysis and Dubuc’s variation analysis) or Hurst exponents (for the variance analysis); these data are shown in Figure 15, with the Hurst exponents “converted” to fractal dimensions via . Plotting these measured parameters as a function of the well-defined spectral exponent used to generate each trace, we see that the relationship breaks down for close to 1 or 2.
7. Generating fractional Brownian motions and characterizing fractal analysis techniques
The framework of the investigation summarized in Figure 15 may be applied to a more thorough investigation of the fidelity of each fractal analysis technique discussed above. That is, if we generate a fBm trace with a well-defined Hurst exponent and subject such a trace to the analysis techniques under consideration, we may evaluate the robustness of each analysis technique. In so doing, we may evaluate not only the fidelity of each analysis method, but also may explore how the analysis methods (individually and/or collectively) respond to less-idealized data sets. That is, by generating fBm traces with well-defined Hurst exponents and modifying the traces to better resemble real-world data sets, we may gain insight into how best to interpret our analytical results of experimentally derived data. Specifically, in addition to testing these analysis techniques on “full-size” 16,384-point fBm traces (with 16,384 arbitrarily chosen as a “sufficiently large” number), we additionally tested these analyses on traces of reduced length and/or reduced spectral content, which may better represent experimentally measured data sets.
A variety of methods exist for generating a fractional Brownian motion trace that exhibits a well-defined predetermined Hurst exponent. Examples of such methods include random midpoint displacement, Fourier filtering of white noise traces, and the summation of independent jumps . This chapter considers randomly generated fBm traces that were created using a MATLAB program that generates a fractional Gaussian noise trace with the desired Hurst exponent via a Fourier transform and subsequently computes the cumulative sum of the noise trace to yield a fractional Brownian motion trace with a specified well-defined Hurst exponent.
While such computer-generated fBm traces are accurately described as exhibiting a well-defined Hurst exponent, the inherently finite nature of these traces precludes the traces from being fully “fractal.” That is, as with any natural structure with finite extent, the generated fBm traces necessarily exhibit a fine-scale resolution limit (owing to the point-wise granularity of the traces) as well as a coarse-scale size limit (owing to the finite total length of the traces). With this in mind, we must be content to forge ahead with the simplifying assumption that the effects of these particular limitations on our estimates of the underlying fractal scaling properties are negligible when considering a computer-generated fBm trace whose total length exceeds its step increment by several orders of magnitude. Accordingly, for the purposes of this analysis, we assume that an fBm trace generated with a predetermined Hurst exponent “” and with a total length well in excess of its resolution limit is a suitable representative of a pure fractal structure characterized by . Thus, we assume that such a trace may fairly be used as a control against which the fidelity of the above-mentioned analysis techniques may be evaluated.
The procedure for evaluating each of these analysis techniques is thus as follows: We first generated a set of 50 16,384-point fBm traces as well as 50 512-point fBm traces at each of 39 input Hurst exponents between 0.025 and 0.975. In this manner, we sought to evaluate not only the fidelity of each fractal analysis technique in returning the expected results for the longer 16,384-point traces, but also the effect of performing the same analyses on data sets of limited length. Next, we applied each analysis technique under consideration to each of these traces, returning either a measured Hurst exponent or a measured fractal dimension . In the case of the Dubuc variation analysis, which returns a measured fractal dimension, this value was “converted”7 to a Hurst exponent via the relation . Having extracted these values of for each sample fBm trace and for each analysis technique, we produced a plot of representing all fBm traces analyzed with each analysis technique; these results are displayed in Figures 16 and 17 for randomly-generated fBm traces with lengths of 16,384 points and 512 points, respectively. In each of Figures 16 and 17, each data point represents the average value measured via the corresponding analysis method. Each corresponding logarithmic scaling plot was fit to a straight line between a fine-scale cutoff of five data points and a coarse-scale cutoff of 1/5 of the full length of the trace. Each error bar represents one standard deviation in the measured values averaged to yield the corresponding data point. The dashed black line represents the ideal relationship ; that is, data points representing traces whose measured values exactly match their generating values would fall on this line.
In the ideal case of a perfectly fractal fBm trace subjected to an analysis technique that produces a precise and accurate value of the Hurst exponent, a plot of vs. is expected to be linear with unity slope. Based on the results of the analyses summarized in Figures 16 and 17, our results may be summarized as follows: the variational box-counting method tends to over-estimate except in the case of high values; the variance analysis tends to under-estimate
We also investigated the effect on the measured
Performing a fractal analysis of time-series traces with limited spectral content requires a reassessment of the length scales over which one expects to observe the fractal scaling properties. Whereas our analysis of fBm traces whose spectral content extended to the resolution limit of the traces examined scaling properties to a minimum length scale of five data points, we now cannot expect to see such scaling properties at length scales smaller than our minimum feature size of 10 data points. Given this well-defined minimum feature size, it may be tempting to set our fine-scale analysis cutoff at 10 data points and expect to observe the desired scaling properties at all length scales greater than this. In practice, however, the effect of such spectral filtering is manifest in a fractal analysis even at length scales significantly greater than that of the minimum feature size.
The results of passing the 512-point Fourier filtered fBm traces through the fractal analysis techniques under consideration are displayed in Figures 19 and 20, which illustrate the results obtained when applying fine-scale cutoffs of 10 data points (i.e., the traces’ minimum feature size) and 20 data points, respectively. In each of Figures 19 and 20, each data point represents the average value measured via the corresponding analysis technique using the aforementioned cutoffs at the fine scale limit and 1/5 of the entire trace as the coarse scale cutoff limit. Each error bar represents one standard deviation in the measured values that were averaged to yield the corresponding data point. The dashed black line represents the ideal relation , as discussed above.
Examples of the logarithmic scaling plots that yielded the data summarized in Figures 16–17 and 19
In each of Figures 21–24, the vertical dashed lines indicate the cutoffs between which the scaling plot is fitted with a straight line whose slope is measured to determine . For both traces in each of these figures, the coarse-scale analysis cutoff corresponds to the location of the line labeled “1/5 of trace.” The fine-scale analysis cutoff for the raw trace (red points) corresponds to the location of the line labeled “5 points” (corresponding to the data in Figure 17), while the fine-scale analysis cutoff for the filtered trace (blue points) may be chosen as 10 data points (corresponding to the data in Figure 19) or 20 data points (corresponding to the data in Figure 20), as represented by respective dashed vertical lines in Figures 21–24.
Contrasting the trends displayed in Figures 19 and 20 with those displayed in Figures 16 and 17 highlights the inherent challenge in assessing the fractal properties of time-series structures that suffer from limited total length and/or limited resolution/spectral content. Indeed, accommodating the impact of a minimum feature size that is significantly in excess of the trace’s resolution limit generally necessitates restricting a fractal analysis to length scales larger still than even this observed minimum feature size. This in turn often restricts an analysis of scaling properties to a consideration of relatively few orders of magnitude in length. For example, performing a fractal analysis of a 512-point Fourier filtered trace using analysis cutoffs corresponding to 10 data points and 1/5 of the trace length corresponds to an analysis of the scaling behavior over barely more than one order of magnitude in length scale; attempting to increase the accuracy of the measurement by raising the fine-scale cutoff to 20 data points further reduces the scaling range to 0.71 orders of magnitude.
Moreover, Figures 21–24 demonstrate the difficulty in identifying an appropriate fine-scale cutoff for fractal analysis of a time-series trace, even when the minimum feature size found in the trace is easily identifiable and/or well-defined. The examples of Figures 21–24 further highlight an important distinction between the application of fractal analysis techniques to spatial and time-series fractals. In the case of spatial fractals, it often is reasonable to expect to observe fractal scaling behavior between the length scales corresponding to physical constraints (and in particular at length scales sufficiently far from these cutoffs). By contrast, and as seen in Figures 21–24, the effect of imposing (or observing) a finite minimum feature size on a time-series trace is evident at
In light of these results, one must take care when applying these analysis techniques to data sets limited in length or spectral content, as it may be difficult to make a compelling argument for the empirical presence of fractal behavior when examining such a narrow range of length scales. Nevertheless, it is instructive to examine the behavior of fractal analysis applied to known fractal structures such as fBm traces that have been artificially subjected to such constraints. For example, one may argue that an fBm trace that is Fourier filtered to exhibit a coarser minimum feature size is analogous to a natural structure or phenomenon that has been subjected to exterior influences such as weathering effects or measurement limits: both may be considered examples of structures that are legitimately generated via processes associated with fractal behavior, but whose true fractal nature has been obfuscated by secondary considerations. In the eyes of the authors, such effects do not necessarily render the resulting structures “less fractal” than their idealized counterparts. Nevertheless, such effects demand careful consideration when choosing an analysis method and an acknowledgment of the inherent limitations thereof.
The authors wish to thank Drs. Adam Micolich, Rick Montgomery, Billy Scannell, and Matthew Fairbanks for fruitful discussions. Generous support for this work was provided by the WM Keck Foundation.
- Though Mandelbrot discusses the concept of fractional dimension in this 1967 paper, he did not introduce the term “fractal” until 1975 .
- While the box-counting method is typically applied to structures embedded in two dimensions, it is straightforward to generalize the technique to higher- or lower-dimensional systems.
- Not to be confused with the variational box-counting method.
- In all discussions of time-series traces, we refer to the independent variable as “time” as a matter of convention unless otherwise specified. Additionally, as a matter of convention, we refer to an interval of the independent variable as a “length” unless otherwise specified.
- Not to be confused with the variational box-counting method or the variance method.
- Note that this relation only applies to time-series fractals, since the notion of a Hurst exponent is undefined for spatial fractals.
- As discussed above, such a conversion is at best an approximation. Nonetheless, utilizing this conversion serves as a self-consistent means of evaluating the response of this analysis technique when applied to fBm traces of a known Hurst exponent, as well as deviations from this behavior.