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		<summary type="html">&lt;p&gt;220.149.255.71: See also : langmuir eqn.&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Karperien Strange Attractor 200.gif|thumb|300px|{{anchor|multifractal}}A [[Strange Attractor]] that exhibits [[multifractal]] scaling]]&lt;br /&gt;
[[File:WF111-Anderson transition-multifractal.jpeg|thumbnail|Example of a multifractal electronic eigenstate at the [[Anderson localization]] transition in a system with 1367631 atoms.]]&lt;br /&gt;
A &#039;&#039;&#039;multifractal system&#039;&#039;&#039; is a generalization of a [[fractal]] system in which a single exponent (the [[fractal dimension]]) is not enough to describe its dynamics; instead, a continuous spectrum of exponents (the so-called [[singularity spectrum]]) is needed.&amp;lt;ref&amp;gt;{{cite book | last = Harte | first = David | title = Multifractals | publisher = Chapman &amp;amp; Hall | location = London | year = 2001 | isbn = 978-1-58488-154-4 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Multifractal systems are common in nature, especially [[geophysics]]. They include [[Turbulence|fully developed turbulence]], [[stock market]] time series, real world scenes, the Sun’s magnetic field time series, [[Cardiac cycle|heartbeat]] dynamics, human gait, and natural luminosity time series.  Models have been proposed in various contexts ranging from turbulence in [[fluid dynamics]] to internet traffic, finance, image modeling, texture synthesis, meteorology, geophysics and more.  The origin of multifractality in sequential (time series) data has been attributed, to mathematical convergence effects related to the [[central limit theorem]] that have as foci of convergence the family of statistical distributions known as the [[Tweedie distributions|&#039;&#039;&#039;Tweedie exponential dispersion models&#039;&#039;&#039;]]&amp;lt;ref name=Kendal2011b&amp;gt;Kendal WS &amp;amp; Jørgensen BR (2011) Tweedie convergence: a mathematical basis for Taylor&#039;s power law, &#039;&#039;1/f&#039;&#039; noise and multifractality. &#039;&#039;Phys. Rev E&#039;&#039; 84, 066120&amp;lt;/ref&amp;gt; as well as the geometric Tweedie models.&amp;lt;ref name=Jørgensen2011&amp;gt; Jørgensen B, Kokonendji CC (2011) Dispersion models for geometric sums. &#039;&#039;Braz J Probab Stat&#039;&#039; 25, 263-293&amp;lt;/ref&amp;gt;  The first convergence effect yields monofractal sequences and the second convergence effect is responsible for variation in the fractal dimension of the monofractal sequences.&amp;lt;ref name=Kendal2014&amp;gt;Kendal WS (2014) Multifractality attributed to dual central limit-lie convergence effects. &#039;&#039;Physica A&#039;&#039; 401, 22-33&amp;lt;/ref&amp;gt;    &lt;br /&gt;
&lt;br /&gt;
From a practical perspective, multifractal analysis uses the mathematical basis of multifractal theory to investigate datasets, often in conjunction with other methods of [[fractal analysis]] and [[lacunarity]] analysis. The technique entails distorting datasets extracted from patterns to generate multifractal spectra that illustrate how scaling varies over the dataset. The [[#techniques|techniques of multifractal analysis]] have been applied in a variety of practical situations such as predicting earthquakes and interpreting medical images.&amp;lt;ref&amp;gt;{{cite pmid|19535282}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;chhabra&amp;quot;&amp;gt;{{cite doi|10.1186/1471-2164-12-506}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite pmid|22101185}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Definition ==&lt;br /&gt;
In a multifractal system &amp;lt;math&amp;gt;s&amp;lt;/math&amp;gt;, the behavior around any point is described by a local [[power law]]:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;s(\vec{x}+\vec{a})-s(\vec{x}) \sim a^{h(\vec{x})}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The exponent &amp;lt;math&amp;gt;h(\vec{x})&amp;lt;/math&amp;gt; is called the [[singularity exponent]], as it describes the local degree of [[Mathematical singularity|singularity]] or [[regularity]]{{disambiguation needed|date=May 2012}} around the point &amp;lt;math&amp;gt;\vec{x}&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The ensemble formed by all the points that share the same singularity exponent is called the &#039;&#039;singularity manifold of exponent h&#039;&#039;, and is a [[fractal set]] of [[fractal dimension]] D(h). The curve D(h) versus h is called the &#039;&#039;singularity spectrum&#039;&#039; and fully describes the (statistical) distribution of the variable &amp;lt;math&amp;gt;s&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
In practice, the multifractal behaviour of a physical system &amp;lt;math&amp;gt;X&amp;lt;/math&amp;gt; is not directly characterized by its singularity spectrum D(h). Data analysis rather gives access to the &#039;&#039;multiscaling exponents&#039;&#039; &amp;lt;math&amp;gt;\zeta(q),\ q\in{\mathbb R}&amp;lt;/math&amp;gt;. Indeed, multifractal signals generally obey a &#039;&#039;scale invariance&#039;&#039; property which yields power law behaviours for multiresolution quantities depending on their scale &amp;lt;math&amp;gt;a&amp;lt;/math&amp;gt;. Depending on the object under study, these multiresolution quantities, denoted by &amp;lt;math&amp;gt;T_X(a)&amp;lt;/math&amp;gt; in the following, can be local averages in boxes of size &amp;lt;math&amp;gt;a&amp;lt;/math&amp;gt;, gradients over distance &amp;lt;math&amp;gt;a&amp;lt;/math&amp;gt;, wavelet coefficients at scale &amp;lt;math&amp;gt;a&amp;lt;/math&amp;gt;... For multifractal objects, one usually observes a global power law scaling of the form:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\langle T_X(a)^q \rangle \sim a^{\zeta(q)}\ &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
at least in some range of scales and for some range of orders &amp;lt;math&amp;gt;q&amp;lt;/math&amp;gt;. When such a behaviour is observed, one talks of scale invariance, self-similarity or multiscaling.&amp;lt;ref&amp;gt;{{cite journal |author=A.J. Roberts and A. Cronin |title=Unbiased estimation of multi-fractal dimensions of finite data sets |journal=Physica A |volume=233 |year=1996 |pages=867–878 |doi=10.1016/S0378-4371(96)00165-3 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Estimation ==&lt;br /&gt;
&lt;br /&gt;
Using the so-called &#039;&#039;multifractal formalism&#039;&#039;, it can be shown that, under some well-suited assumptions, there exists a correspondence between the singularity spectrum &amp;lt;math&amp;gt;D(h)&amp;lt;/math&amp;gt; and the multiscaling exponents &amp;lt;math&amp;gt;\zeta(q)&amp;lt;/math&amp;gt; through a [[Legendre transform]]. While the determination of &amp;lt;math&amp;gt;D(h)&amp;lt;/math&amp;gt; calls for some exhaustive local analysis of the data, which would result in difficult and numerically unstable calculations, the estimation of the &amp;lt;math&amp;gt;\zeta(q)&amp;lt;/math&amp;gt; relies on the use of statistical averages and linear regressions in log-log diagrams. Once the &amp;lt;math&amp;gt;\zeta(q)&amp;lt;/math&amp;gt; are known, one can deduce an estimate of &amp;lt;math&amp;gt;D(h)&amp;lt;/math&amp;gt; thanks to a simple Legendre transform.&lt;br /&gt;
&lt;br /&gt;
Multifractal systems are often modeled by stochastic processes such as [[multiplicative cascade]]s. Interestingly, the &amp;lt;math&amp;gt;\zeta(q)&amp;lt;/math&amp;gt; receives some statistical interpretation as they characterize the evolution of the distributions of the &amp;lt;math&amp;gt;T_X(a)&amp;lt;/math&amp;gt; as &amp;lt;math&amp;gt;a&amp;lt;/math&amp;gt; goes from larger to smaller scales. This evolution is often called &#039;&#039;statistical intermittency&#039;&#039; and betrays a departure from [[Gaussian]] models.&lt;br /&gt;
&lt;br /&gt;
Modelling as a [[multiplicative cascade]] also leads to estimation of multifractal properties for relatively small datasets ({{harvnb|Roberts|Cronin|1996}}).  A maximum likelihood fit of a multiplicative cascade to the dataset not only estimates the complete spectrum, but also gives reasonable estimates of the errors (see the web service [http://www.maths.adelaide.edu.au/anthony.roberts/multifractal.php]).&lt;br /&gt;
&lt;br /&gt;
{{anchor|techniques}}&lt;br /&gt;
&lt;br /&gt;
== Practical application of multifractal spectra ==&lt;br /&gt;
[[File:Distort.gif|thumb|Multifractal analysis is analogous to viewing a dataset through a series of distorting lenses to home in on differences in scaling. The pattern shown is a [[Hénon map]]]]&lt;br /&gt;
&lt;br /&gt;
{{anchor|distort}}Multifractal analysis has been used in several fields in science to characterize various types of datasets.&amp;lt;ref&amp;gt;{{cite doi|10.1364/OE.20.003015}}&amp;lt;/ref&amp;gt; In essence, multifractal analysis applies a distorting factor to datasets extracted from patterns, to compare how the data behave at each distortion. This is done using graphs known as &#039;&#039;&#039;multifractal spectra&#039;&#039;&#039; that illustrate how the distortions affect the data, analogous to viewing the dataset through a &amp;quot;distorting lens&amp;quot; as shown in the [[#distort|illustration]].&amp;lt;ref name=&amp;quot;bcmf&amp;quot;/&amp;gt;  Several types of multifractal spectra are used in practise.&lt;br /&gt;
&lt;br /&gt;
=== D&amp;lt;sub&amp;gt;Q&amp;lt;/sub&amp;gt; vs Q ===&lt;br /&gt;
{{anchor|dqvsq}}[[File:Dqvsq.gif|thumb|D&amp;lt;sub&amp;gt;Q&amp;lt;/sub&amp;gt; vs Q spectra for a non-fractal circle (empirical box counting dimension = 1.0), mono-fractal [[List of fractals by Hausdorff dimension#cross|Quadric Cross]] (empirical box counting dimension = 1.49), and multifractal [[Hénon map]] (empirical box counting dimension = 1.29).]]&lt;br /&gt;
&lt;br /&gt;
{{anchor|dimensional ordering}}One practical multifractal spectrum is the graph of D&amp;lt;sub&amp;gt;Q&amp;lt;/sub&amp;gt; vs Q, where D&amp;lt;sub&amp;gt;Q&amp;lt;/sub&amp;gt; is the &#039;&#039;&#039;generalized dimension&#039;&#039;&#039; for a dataset and Q is an arbitrary set of exponents. The expression &#039;&#039;generalized dimension&#039;&#039; thus refers to a set of dimensions for a dataset (detailed calculations for determining the generalized dimension using [[box counting]] are described [[#generalized dimension|below]]).&lt;br /&gt;
&lt;br /&gt;
==== Dimensional ordering ====&lt;br /&gt;
The general pattern of the graph of D&amp;lt;sub&amp;gt;Q&amp;lt;/sub&amp;gt; vs Q can be used to assess the scaling in a pattern.  The graph is generally decreasing, sigmoidal around Q=0, where D&amp;lt;sub&amp;gt;(Q=0)&amp;lt;/sub&amp;gt; ≥ D&amp;lt;sub&amp;gt;(Q=1)&amp;lt;/sub&amp;gt; ≥ D&amp;lt;sub&amp;gt;(Q=2)&amp;lt;/sub&amp;gt;. As illustrated in the [[#dqvsq|figure]], variation in this graphical spectrum can help distinguish patterns. The image shows D&amp;lt;sub&amp;gt;(Q)&amp;lt;/sub&amp;gt; spectra from a multifractal analysis of binary images of non-, mono-, and multi-fractal sets. As is the case in the sample images, non- and mono-fractals tend to have flatter D&amp;lt;sub&amp;gt;(Q)&amp;lt;/sub&amp;gt; spectra than multifractals. &lt;br /&gt;
&lt;br /&gt;
The generalized dimension also offers some important specific information. D&amp;lt;sub&amp;gt;(Q=0)&amp;lt;/sub&amp;gt; is equal to the [[Capacity Dimension]], which in the analysis shown in the figures here is the [[box counting dimension]]. D&amp;lt;sub&amp;gt;(Q=1)&amp;lt;/sub&amp;gt; is equal to the [[Information Dimension]], and D&amp;lt;sub&amp;gt;(Q=2)&amp;lt;/sub&amp;gt; to the [[Correlation Dimension]]. This relates to the &amp;quot;multi&amp;quot; in multifractal whereby multifractals have multiple dimensions in the D&amp;lt;sub&amp;gt;(Q)&amp;lt;/sub&amp;gt; vs Q spectra but monofractals stay rather flat in that area.&amp;lt;ref name=&amp;quot;bcmf&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;chaabra&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== &amp;lt;math&amp;gt;f(\alpha)&amp;lt;/math&amp;gt; vs &amp;lt;math&amp;gt;\alpha&amp;lt;/math&amp;gt; ===&lt;br /&gt;
Another useful multifractal spectrum is the graph of &amp;lt;math&amp;gt;f(\alpha)&amp;lt;/math&amp;gt; vs &amp;lt;math&amp;gt;\alpha&amp;lt;/math&amp;gt; (see [[#calculations|calculations]]). These graphs generally rise to a maximum that approximates the [[fractal dimension]] at Q=0, and then fall. Like D&amp;lt;sub&amp;gt;Q&amp;lt;/sub&amp;gt; vs Q spectra, they also show typical patterns useful for comparing non-, mono-, and multi-fractal patterns. In particular, for these spectra, non- and mono-fractals converge on certain values, whereas the spectra from multifractal patterns are typically humped over a broader extent.&lt;br /&gt;
&lt;br /&gt;
== Estimating multifractal scaling from box counting ==&lt;br /&gt;
{{anchor|calculations}}&lt;br /&gt;
Multifractal spectra can be determined from [[box counting]] on digital images. First, a box counting scan is done to determine how the pixels are distributed; then, this &amp;quot;mass distribution&amp;quot; becomes the basis for a series of calculations.&amp;lt;ref name=&amp;quot;bcmf&amp;quot;&amp;gt;{{citation | author=Karperien, A |title=What are Multifractals? | publisher=ImageJ | accessdate=2012-02-10|url=http://rsbweb.nih.gov/ij/plugins/fraclac/FLHelp/Multifractals.htm |year=2002 |archive=http://www.webcitation.org/65LENzkV8}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;chaabra&amp;quot;&amp;gt;{{cite doi|10.1103/PhysRevLett.62.1327}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite doi|10.2136/sssaj2001.6551361x}}&amp;lt;/ref&amp;gt; The chief idea is that for multifractals, the probability, &amp;lt;math&amp;gt;P&amp;lt;/math&amp;gt;, of a number of pixels, &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt;, appearing in a box, &amp;lt;math&amp;gt;i&amp;lt;/math&amp;gt;, varies as box size, &amp;lt;math&amp;gt;\textstyle\epsilon&amp;lt;/math&amp;gt;, to some exponent, &amp;lt;math&amp;gt;\textstyle\alpha&amp;lt;/math&amp;gt;, which changes over the image, as in {{EquationNote|Eq.0.0}}. &#039;&#039;NB: For mono[[fractals]], in contrast, the exponent does not change meaningfully over the set.&#039;&#039; &amp;lt;math&amp;gt;P&amp;lt;/math&amp;gt; is calculated from the box counting pixel distribution as in {{EquationNote|Eq.2.0}}. &lt;br /&gt;
 &lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;P_{[i,\epsilon]} \varpropto \epsilon^{-\alpha_i} \therefore\alpha_i \varpropto \frac{\log{P_{[i,\epsilon]}}}{\log{\epsilon^{-1}}}&amp;lt;/math&amp;gt;|{{EquationRef|Eq.0.0}}}}&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt; = an arbitrary scale ([[Box counting|box size]] in box counting) at which the set is examined&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;i&amp;lt;/math&amp;gt; = the index for each box laid over the set for an &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;m_{[i,\epsilon]}&amp;lt;/math&amp;gt; = the number of pixels or &#039;&#039;mass&#039;&#039; in any box, &amp;lt;math&amp;gt;i&amp;lt;/math&amp;gt;, at size &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;N_\epsilon&amp;lt;/math&amp;gt; = the total boxes that contained more than 0 pixels, for each &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;M_\epsilon = \sum_{i=1}^{N_\epsilon}m_{[i,\epsilon]} = &amp;lt;/math&amp;gt; the total mass or sum of pixels in all boxes for this &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;|{{EquationRef|Eq.1.0}}}} &lt;br /&gt;
&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;P_{[i,\epsilon]} = \frac{m_{[i,\epsilon]}}{M_\epsilon} = &amp;lt;/math&amp;gt; the probability of this mass at &amp;lt;math&amp;gt;i&amp;lt;/math&amp;gt; relative to the total mass for a box size|{{EquationRef|Eq.2.0}}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;P&amp;lt;/math&amp;gt; is used to observe how the pixel distribution behaves when distorted in certain ways as in {{EquationNote|Eq.3.0}} and {{EquationNote|Eq.3.1}}:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; = an arbitrary range of values to use as exponents for distorting the data set&lt;br /&gt;
&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;I_{{(Q)}_{[\epsilon]}} = \sum_{i=1}^{N_\epsilon} {P_{[i,\epsilon]}^Q} = &amp;lt;/math&amp;gt; the sum of all mass probabilities distorted by being raised to this Q, for this box size|{{EquationRef |Eq.3.0}}}}&lt;br /&gt;
:*When &amp;lt;math&amp;gt;Q=1&amp;lt;/math&amp;gt;, {{EquationNote|Eq.3.0}} equals 1, the usual sum of all probabilities, and when &amp;lt;math&amp;gt;Q=0&amp;lt;/math&amp;gt;, every term is equal to 1, so the sum is equal to the number of boxes counted, &amp;lt;math&amp;gt;N_\epsilon&amp;lt;/math&amp;gt;.&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;\mu_{{(Q)}_{[i,\epsilon]}} = \frac{P_{[i,\epsilon]}^Q}{I_{{(Q)}_{[\epsilon]}}} = &amp;lt;/math&amp;gt; how the distorted mass probability at a box compares to the distorted sum over all boxes at this box size|{{EquationRef|Eq.3.1}}}}&lt;br /&gt;
&lt;br /&gt;
These distorting equations are further used to address how the set behaves when scaled or resolved or cut up into a series of &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;-sized pieces and distorted by Q, to find different values for the dimension of the set, as in the following:&lt;br /&gt;
&lt;br /&gt;
:*An important feature of {{EquationNote|Eq.3.0}} is that it can also be seen to vary according to scale raised to the exponent &amp;lt;math&amp;gt;\textstyle\tau&amp;lt;/math&amp;gt; in {{EquationNote|Eq.4.0}}:&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;I_{{(Q)}_{[\epsilon]}} \varpropto \epsilon^{\tau_{(Q)}}&amp;lt;/math&amp;gt;|{{EquationRef|Eq.4.0}}}}&lt;br /&gt;
&lt;br /&gt;
Thus, a series of values for &amp;lt;math&amp;gt;\tau_{(Q)} &amp;lt;/math&amp;gt; can be found from the slopes of the regression line for the log of {{EquationNote|Eq.3.0}} vs the log of &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt; for each &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;, based on {{EquationNote|Eq.4.1}}:&lt;br /&gt;
&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;\tau_{(Q)} = {\lim_{\epsilon\to0}{\left[ \frac {ln{I_{{(Q)}_{[\epsilon]}}}} {ln{\epsilon}} \right ]}} &amp;lt;/math&amp;gt;|{{EquationRef|Eq.4.1}}}}&lt;br /&gt;
 &lt;br /&gt;
:*{{anchor|generalized dimension}}For the generalized dimension:&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;D_{(Q)} = {\lim_{\epsilon\to0} { \left [ \frac{ln{I_{{(Q)}_{[\epsilon]}}}}{ln{\epsilon^{-1}}} \right ]}} {(1-Q)^{-1}} &amp;lt;/math&amp;gt;|{{EquationRef|Eq.5.0}}}}&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;D_{(Q)} = \frac{\tau_{(Q)}}{Q-1}&amp;lt;/math&amp;gt;|{{EquationRef|Eq.5.1}}}} &lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;\tau_{{(Q)}_{}} = D_{(Q)}\left(Q-1\right)&amp;lt;/math&amp;gt;|{{EquationRef|Eq.5.2}}}}&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;\tau_{(Q)} = \alpha_{(Q)}Q - f_{\left(\alpha_{(Q)}\right)}&amp;lt;/math&amp;gt;|{{EquationRef|Eq.5.3}}}}&lt;br /&gt;
&lt;br /&gt;
:*&amp;lt;math&amp;gt;\textstyle\alpha_{(Q)}&amp;lt;/math&amp;gt; is estimated as the slope of the regression line for {{math|log A&amp;lt;sub&amp;gt;&amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;,Q&amp;lt;/sub&amp;gt;}} vs {{math|log &amp;lt;math&amp;gt;\epsilon&amp;lt;/math&amp;gt;}} where:&lt;br /&gt;
&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;A_{\epsilon,Q} =  \sum_{i=1}^{N_\epsilon}{\mu_{{i,\epsilon}_{Q}}{P_{{i,\epsilon}_{Q}}}} &amp;lt;/math&amp;gt;|{{EquationRef|Eq.6.0}}}}&lt;br /&gt;
:*Then &amp;lt;math&amp;gt;f_{\left(\alpha_{{(Q)}}\right)}&amp;lt;/math&amp;gt; is found from {{EquationNote|Eq.5.3}}.&lt;br /&gt;
&lt;br /&gt;
:*The mean &amp;lt;math&amp;gt;\textstyle\tau_{(Q)}&amp;lt;/math&amp;gt; is estimated as the slope of the log-log regression line for &amp;lt;math&amp;gt;\textstyle\tau_{{(Q)}_{[\epsilon]}}&amp;lt;/math&amp;gt; vs &amp;lt;math&amp;gt;\textstyle\epsilon&amp;lt;/math&amp;gt;, where:&lt;br /&gt;
&lt;br /&gt;
{{NumBlk|:|&amp;lt;math&amp;gt;\tau_{(Q)_{[\epsilon]}} = \frac{\sum_{i=1}^{N_\epsilon} {P_{[i,\epsilon]}^{Q-1}}}  {N_\epsilon} &amp;lt;/math&amp;gt;|{{EquationRef|Eq.6.1}}}}&lt;br /&gt;
&lt;br /&gt;
In practise, the probability distribution depends on how the dataset is sampled, so optimizing algorithms have been developed to ensure adequate sampling.&amp;lt;ref name=&amp;quot;bcmf&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* [[Multifractal Model of Asset Returns]] (MMAR)&lt;br /&gt;
* [[Multifractal Random Walk model]] (MRW)&lt;br /&gt;
* [[Fractional Brownian motion]]&lt;br /&gt;
* [[Mandelbrot cascade]], [[continuous cascade]] and [[lognormal cascade]]&lt;br /&gt;
* [[Detrended fluctuation analysis]]&lt;br /&gt;
* [[Tweedie distributions]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
&amp;lt;references /&amp;gt;&lt;br /&gt;
:11. Veneziano, D. and Essiam, A.K. (2003). Flow through porous media with multifractal hydraulic conductivity. &lt;br /&gt;
:Water Resources Research 39: doi: 10.1029/2001WR001018. issn: 0043-1397.&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
*{{cite journal |author=Stanley H.E., Meakin P. |title=Multifractal phenomena in physics and chemistry |journal=Nature |volume=335 |year=1988 |pages=405–9 |url=http://polymer.bu.edu/hes/articles/sm88.pdf |format=Review |doi=10.1038/335405a0 |issue=6189}}&lt;br /&gt;
&lt;br /&gt;
*{{cite journal |author=Alain Arneodo, &#039;&#039;et al.&#039;&#039; |title=Wavelet-based multifractal analysis |journal=Scholarpedia |volume=3 |issue=3 |pages=4103 |year=2008 |url=http://www.scholarpedia.org/article/Wavelet-based_multifractal_analysis |doi=10.4249/scholarpedia.4103}}&lt;br /&gt;
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* [http://www2.warwick.ac.uk/fac/sci/physics/research/theory/research/disqs/media Movies of visualizations of multifractals]&lt;br /&gt;
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{{Fractals}}&lt;br /&gt;
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{{DEFAULTSORT:Multifractal System}}&lt;br /&gt;
[[Category:Fractals]]&lt;br /&gt;
[[Category:Dimension theory]]&lt;/div&gt;</summary>
		<author><name>220.149.255.71</name></author>
	</entry>
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