<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">ACS</journal-id><journal-title-group><journal-title>Atmospheric and Climate Sciences</journal-title></journal-title-group><issn pub-type="epub">2160-0414</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/acs.2015.54036</article-id><article-id pub-id-type="publisher-id">ACS-60565</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Characterization of the Atmospheric Dynamics in Riobamba City Using the Chaos Theory
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>rquímides</surname><given-names>Haro</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Cecilia</surname><given-names>Limaico</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yolanda</surname><given-names>Llosas</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Faculty of Engineering, National University of Chimborazo, Riobamba, Ecuador</addr-line></aff><aff id="aff1"><addr-line>Physics and Mathematics School, Polytechnic School of Chimborazo, Riobamba, Ecuador</addr-line></aff><aff id="aff3"><addr-line>Department of Automatic Control, East University, Santiago, Cuba</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>arquimidesharo@yahoo.es(RH)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>14</day><month>09</month><year>2015</year></pub-date><volume>05</volume><issue>04</issue><fpage>441</fpage><lpage>449</lpage><history><date date-type="received"><day>30</day>	<month>June</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>23</month>	<year>October</year>	</date><date date-type="accepted"><day>26</day>	<month>October</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Chaos studies all that is messy, disorganized and incoherent; mathematically the chaos is a dynamic system governed by nonlinear differential equations. Chaos has an unpredictable behavior; its dynamical is very sensitive to the initial conditions. Atypical chaotic system is the atmosphere; this limits the knowledge about its behavior; but with the advance in the computers, the results that are obtained with the chaos theory improved significantly; the description of atmosphera and its results have extended to other fields of the science, as the economy, health and others. The object of this work was to determine the atmospheric dynamics in the Riobamba city using the theory of chaos, with meteorological data of the meteorological station of the ESPOCH of one year (2010) of data that were processed with model TISEAN. The results determine a hyperchaotic system, according to the coefficients of Lyapunov.
 
</p></abstract><kwd-group><kwd>Chaos Theory</kwd><kwd> Atmospheric Variables</kwd><kwd> Coefficients of Lyapunov</kwd><kwd> Dynamics</kwd><kwd> Entropy</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Chaos and the fractals are part of a bigger topic, dynamics. Dynamics began by the middle of 1600, when Isaac Newton invented the differential equations; he discovered the movement laws and the general gravitation. The following generations of mathematical and physicist treated problems of three bodies, but they realized that they were much more difficult than the problem of two bodies, until the point of considering them impossible [<xref ref-type="bibr" rid="scirp.60565-ref1">1</xref>] .</p><p>The history of chaos begins when the high-speed computers were invented (1950). In 1963 Edwar Lorenz worked in some equations (the equations worldwide well-known as equations of Lorenz) that predicted the time in the atmosphere, and he saw the behavior of its equations graphically. Although they were called high-speed computers in this time, now they are very slow [<xref ref-type="bibr" rid="scirp.60565-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.60565-ref3">3</xref>] .</p><p>The 1970s was the boom of chaos. In 1971, David Ruelle and Takias proposed a new theory for the turbulence of fluids based on a strange attractor. Years later they found case examples in repeated maps of population. He discovered that there are specific universal laws that differentiate the transition between regular behavior and chaos. That is, if it is possible that two systems evolve in a chaotic behavior like.</p><p>This work has taken a set of meteorological data (meteorological station, ESPOCH, 2010), which are pro- cessed, beginning with noise reduction, then, it determined the delay coordinates, the embedding parameters, which help determine the reconstruction of data in the space of the phases, to establish its dynamic estimated coefficients of Lyapunov, fractal dimension and entropy was also to do a prediction of the data based on the characteristics found and an analysis of actual and predicted data.</p></sec><sec id="s2"><title>2. Material and Methods</title><sec id="s2_1"><title>2.1. Chaos Theory</title><p>Chaos theory is a field of study of the mathematics. It studies the behavior of dynamical systems that are highly sensitive to the initial conditions. Small differences in initial conditions (such as those due to rounding errors in numerical computation) this produce in diverging outcomes for such systems dynamic, it does long-term predictions impossibles [<xref ref-type="bibr" rid="scirp.60565-ref4">4</xref>] .</p></sec><sec id="s2_2"><title>2.2. Dynamical Systems</title><p>A dynamic system can be represented by ordinary differential equations, Equation (1).</p><disp-formula id="scirp.60565-formula2207"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x5.png"  xlink:type="simple"/></disp-formula><p>or in discrete time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x6.png" xlink:type="simple"/></inline-formula> by maps of the form, Equation (2).</p><disp-formula id="scirp.60565-formula2208"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x7.png"  xlink:type="simple"/></disp-formula><p>However, chaotic systems do not respond to these equations, but now is possible to use the chaos theory; it follows procedures that go: from the reconstruction of the data series to the phases space, the determination of the degree of chaos and reaching the prediction of the systems [<xref ref-type="bibr" rid="scirp.60565-ref5">5</xref>] .</p></sec><sec id="s2_3"><title>2.3. Delay Coordinates</title><p>A time series can then be thought of as a sequence of observations<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x8.png" xlink:type="simple"/></inline-formula>. Since the (usually scalar) sequence <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x9.png" xlink:type="simple"/></inline-formula> in itself does not properly represent the (multidimensional) phase space of the dynamical system, one has to employ some technique to determine the multidimensional structure of the data.</p><p>The most important phase space reconstruction technique is the method of delays. Vectors in a new space, the embedding space, are formed from time delayed values of the scalar measurements, Equation (3):</p><disp-formula id="scirp.60565-formula2209"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x10.png"  xlink:type="simple"/></disp-formula><p>The number m of elements is called the embedding dimension; the time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x11.png" xlink:type="simple"/></inline-formula> is generally referred to as the delay or lag. Celebrated embedding theorems by Takens [<xref ref-type="bibr" rid="scirp.60565-ref6">6</xref>] and by Sauer et al. [<xref ref-type="bibr" rid="scirp.60565-ref7">7</xref>] state that if the sequence <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x12.png" xlink:type="simple"/></inline-formula> does indeed consist of scalar measurements of the state of a dynamical system, then under certain genericity assumptions, the time delay embedding provides a one-to-one image of the original set<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x13.png" xlink:type="simple"/></inline-formula>, provided m is large enough.</p><p>Time delay embedding is used in almost all methods described [<xref ref-type="bibr" rid="scirp.60565-ref4">4</xref>] . The implementation is straightforward and does not require further explanation. If N scalar measurements are available, the number of embedding vectors are<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x14.png" xlink:type="simple"/></inline-formula>. This has to be kept in mind for the correct normalization of averaged quantities. There is a large literature on the “optimal” choice of the embedding parameters m and τ. These results provide the applied software.</p></sec><sec id="s2_4"><title>2.4. Embedding Parameters</title><p>A method to determine the minimal sufficient embedding dimension m was proposed by Kennel et al. [<xref ref-type="bibr" rid="scirp.60565-ref8">8</xref>] . It is called the false nearest neighbor method. The idea is quite intuitive. Suppose the minimal embedding dimension for a given time series <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x15.png" xlink:type="simple"/></inline-formula> is m<sub>0</sub>. This means that in a m<sub>0</sub> dimensional delay space the reconstructed attractor is a one-to-one image of the attractor in the original phase space. Especially, the topological properties are preserved. Thus the neighbors of a given point are mapped onto neighbors in the delay space. Due to the assumed smoothness of the dynamics, neighborhoods of the points are mapped onto neighborhoods again. Of course the shape and the diameter of the neighborhoods is changed according to the Lyapunov exponents. But suppose now you embed in an m-dimensional space with m &lt; m<sub>0</sub>. Due to this projection the topological structure is not longer preserved. Points are projected into neighborhoods of other points to which they wouldn't belong in higher dimensions. These points are called false neighbors. If now the dynamic is applied, these false neighbors are not typically mapped into the image of the neighborhood, but somewhere else, so that the average “diameter” becomes quite large [<xref ref-type="bibr" rid="scirp.60565-ref6">6</xref>] .</p><p>The idea of the algorithm false_nearest is the following. For each point <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x16.png" xlink:type="simple"/></inline-formula> in the time series look for its nearest neighbor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x17.png" xlink:type="simple"/></inline-formula> in am-dimensional space. Calculate the distance<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x18.png" xlink:type="simple"/></inline-formula>. Iterate both points and compute, Equation (4).</p><disp-formula id="scirp.60565-formula2210"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x19.png"  xlink:type="simple"/></disp-formula><p>If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x20.png" xlink:type="simple"/></inline-formula> exceeds a given heuristic threshold<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x21.png" xlink:type="simple"/></inline-formula>, this point is marked as having a false nearest neighbor [<xref ref-type="bibr" rid="scirp.60565-ref9">9</xref>] . The criterion that the embedding dimension is high enough is that the fraction of points for which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x22.png" xlink:type="simple"/></inline-formula> is zero, or at least sufficiently small. Two examples are shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>. One is for the Lorenz system (crosses), one for the H&#233;non system (filled circles), and one for a H&#233;non time series corrupted by 10% of Gaussian white noise (open circles). One clearly sees that, as expected, m = 2 is sufficient for the H&#233;non and m = 3 for the Lorenz system, whereas the signature is less clear in the noisy case, <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>The introduction of the false nearest neighbors concept and other ad hoc instruments was partly a reaction to the finding that many results obtained for the genuine invariants, like the correlation dimension, has been spurious due to caveats of the estimation procedure. In the latter case, serial correlations and small sample fluctuations can easily be mistaken for nonlinear determinism. It turns out, however, that the ad hoc quantities basically suffer from the same problems―which can be cured by the same precautions. The implementation false_nearest therefore allows to specify a minimal temporal separation of valid neighbors.</p></sec><sec id="s2_5"><title>2.5. Attractor</title><p>The attractor of a dynamic system is the region of space of the phases, in which the path is drawn, tending the movement after a time of adjustment to the attractor. A vast class of dissipative dynamical systems, has the re-</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> The fraction of false nearest neighbors as a function of the embedding dimension for noise free Lorenz (blue) and H&#233;non (red) time series, as well as a H&#233;non time series (green) corrupted by 10% of noise</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x23.png"/></fig><p>markable property of possessing an attractor, which is the place of routes after a long enough career points. A simple example is that of the pendulum swinging in the air, the amplitude of oscillation is progressively attenuated and all paths regardless of the initial conditions are approaching stable fixed point which is the attractor [<xref ref-type="bibr" rid="scirp.60565-ref10">10</xref>] .</p><p>In the case of chaotic systems, in which it has a strong dependence of the initial coordinates, the attractor is not in fact a regular object, but rather has a very complicated structure, then called him strange attractor (Rulle) [<xref ref-type="bibr" rid="scirp.60565-ref11">11</xref>] , which can have a fractal structure.</p></sec><sec id="s2_6"><title>2.6. Noise Reduction</title><p>This noise reduction scheme is implemented quite easily. First an embedding has to be chosen. Except for extremely oversampled data, it is advantageous to choose a short time delay. The program always uses unit delay. The embedding dimension m should be chosen somewhat higher than that required by the embedding theorems. Then for each embedding vector {S<sub>n</sub>}, a neighborhood <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x24.png" xlink:type="simple"/></inline-formula> is formed in phase space containing all points <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x25.png" xlink:type="simple"/></inline-formula> such as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x26.png" xlink:type="simple"/></inline-formula>. The radius of the neighborhoods ɛ should be taken large enough in order to cover the noise extent, but still smaller than a typical curvature radius. These conditions cannot always be fulfilled simultaneously, in which case one has to repeat the process with several choices and carefully evaluate the results. If the noise level is substantially smaller than the typical radius of curvature, neighborhoods of radius about 2 - 3 times the noise level gave the best results with artificial data. For each embedding vector <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x27.png" xlink:type="simple"/></inline-formula> (the delay time has been set to unity), a corrected middle coordinate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x28.png" xlink:type="simple"/></inline-formula> is computed by averaging over the neighborhood, Equation (5):</p><disp-formula id="scirp.60565-formula2211"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x29.png"  xlink:type="simple"/></disp-formula><p>Then complete around the series of time, all the measures <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x30.png" xlink:type="simple"/></inline-formula> are remplazadas for the correct values<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x31.png" xlink:type="simple"/></inline-formula>, according to the first and the next (m − 1)/2 points, if m is strange the correction is not valid, the half correction can be taken as a new radio of neighboring reinforcements for the next interaction [<xref ref-type="bibr" rid="scirp.60565-ref12">12</xref>] .</p></sec><sec id="s2_7"><title>2.7. Lyapunov Exponents</title><p>Chaos arises from the exponential growth of infinitesimal perturbations, together with global folding mechanisms to guarantee boundedness of the solutions. This exponential instability is characterized by the spectrum of Lyapunov exponents [<xref ref-type="bibr" rid="scirp.60565-ref13">13</xref>] . If one assumes a local decomposition of the phase space into directions with different stretching or contraction rates, then the spectrum of exponents is the proper average of these local rates over the whole invariant set, and thus consists of as many exponents as there are space directions. The most prominent problem in time series analysis is that the physical phase space is unknown, and that instead the spectrum is computed in some embedding space. Thus the number of the exponents depends on the reconstruction, and might be larger than in the physical phase space.</p><p>Chaos arises of the exponential growth of the infinitesimal interferences, the exponents of Lyapunov (λ) that quantify are to guarantee the analysis of this uncertainty as much as they go away two trajectories [<xref ref-type="bibr" rid="scirp.60565-ref14">14</xref>] .</p><disp-formula id="scirp.60565-formula2212"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x32.png"  xlink:type="simple"/></disp-formula><p>With l(t) semi axis bigger than an ellipse, r small radio initial and t big time, in general settles down:</p><disp-formula id="scirp.60565-formula2213"><graphic  xlink:href="http://html.scirp.org/file/9-4700296x33.png"  xlink:type="simple"/></disp-formula><p>Variables that allow to characterizing an attractor, this way:</p><p>a) For a fixed point the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x34.png" xlink:type="simple"/></inline-formula> are negative.</p><p>b) In a cycle limit <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x35.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x36.png" xlink:type="simple"/></inline-formula> for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x37.png" xlink:type="simple"/></inline-formula>.</p><p>c) In the movement of a dimensional Torous n, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x38.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x39.png" xlink:type="simple"/></inline-formula> for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x40.png" xlink:type="simple"/></inline-formula>.</p><p>d) In a chaotic system at least one Lyapunov exponent is negative.</p><p>The computation of the full Lyapunov spectrum requires considerably more effort than just the maximal exponent. An essential ingredient is some estimate of the local Jacobians, i.e. of the linearized dynamics, which rules the growth of infinitesimal perturbations. One either finds it from direct fits of local linear models of the type<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x41.png" xlink:type="simple"/></inline-formula>, such as the first row of the Jacobian is the vector a<sub>n</sub>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x42.png" xlink:type="simple"/></inline-formula> for i = 2,…, mi = 2, where m is the embedding dimension. The a<sub>n</sub> is given by the last squares minimization <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-4700296x43.png" xlink:type="simple"/></inline-formula> where S<sub>l</sub> is the set neighbors of S<sub>n</sub> [<xref ref-type="bibr" rid="scirp.60565-ref6">6</xref>] .</p><p>From this result can define Kolmogorov entropy-Sinai.</p><disp-formula id="scirp.60565-formula2214"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x44.png"  xlink:type="simple"/></disp-formula><p>Or the dimension fractal of Kaplan. Yorke (1979)</p><disp-formula id="scirp.60565-formula2215"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x45.png"  xlink:type="simple"/></disp-formula><p>With j positive Lyapunov coefficients [<xref ref-type="bibr" rid="scirp.60565-ref5">5</xref>] .</p></sec><sec id="s2_8"><title>2.8. Predicting Time Series</title><p>The basic functions used are Gaussians, with center points chosen to be data from the time series. The variance of Gaussians are set to the average distance between the centers [<xref ref-type="bibr" rid="scirp.60565-ref15">15</xref>] .</p><p>The pattern predicts the series of data using the following relationship:</p><disp-formula id="scirp.60565-formula2216"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-4700296x46.png"  xlink:type="simple"/></disp-formula><p>where x<sub>n</sub> is the n-th delay vector and f<sub>i</sub> is a gaussian centered at the i-th center point and a constants.</p></sec><sec id="s2_9"><title>2.9. Atmospheric Dynamics</title><p>The atmospheric time, besides being a dynamic system, is very sensitive to the changes in the initial variables, it is a transitive system and its periodic orbits are also dense, that makes of it an appropriate system to work with chaotic mathematics. The precision of the meteorological predictions is relative, and the announced percentages have not much meaning without a detailed description of the approaches used to judge the accuracy of the prediction.</p><p>Before the appearance of the Theory of Chaos, it was thought that the climate ended up being predicted with a Newton like accuracy. It was not more than a matter of introducing variables more and more in a computer sufficiently potent to process them. However, of some few variables of only some decades ago, now, they has considerate hundreds of thousands of variables without getting the prospective predictability, recently it has been proven that the chaotic character of the atmospheric time has to do with the geometric properties group of evolution of the climatic terrestrial system. These results suggest a practical impossibility to predict weather in the medium and long term. The climate is sensitive to small variations in the initial conditions and the determination of the initial conditions exactly is doomed to failure because of the Heisenberg uncertainty principle. In these days it is possible to demonstrate the dependability of the predictions with the theory of chaos for periods of up to five days thanks to the density among the periodic orbits of the system, and some successes have been achieved in the prediction of abnormal variations of some variables for periods of up to 30 days [<xref ref-type="bibr" rid="scirp.60565-ref15">15</xref>] .</p></sec></sec><sec id="s3"><title>3. Results and Discussion</title><sec id="s3_1"><title>3.1. Calculation of the Delay Time and Embedding Dimension</title><p>To perform the calculation has been used TISIAN model, in first instance you proceeds to determine the time of retard to reconstruct the series of meteorological data taken in the space of the phases and the embedding dimensions for to data series with noise reduction (<xref ref-type="table" rid="table1">Table 1</xref>).</p></sec><sec id="s3_2"><title>3.2. Calculation of the Spectrum of Lyapunov</title><p>In each case (<xref ref-type="fig" rid="fig2">Figure 2</xref>), it is observed that there are two coefficients of Lyapunov that which indicates that the system is hypercaotic, the precipitation series he/she didn't also find correlation among the data for what you could not determine these coefficients.</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Graph of the spectrum of Lyapunov of the meteorological data with noise reduction</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x47.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Determined delay time (first minimum) function for the different parameters</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Parameter</th><th align="center" valign="middle" >Delay Time</th><th align="center" valign="middle" >Ebedding Dimention</th></tr></thead><tr><td align="center" valign="middle" >Temperature</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >21</td></tr><tr><td align="center" valign="middle" >Humidity</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >10</td></tr><tr><td align="center" valign="middle" >Wind Speed</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >25</td></tr><tr><td align="center" valign="middle" >Precipitation</td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >16</td></tr><tr><td align="center" valign="middle" >Pressure</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >7</td></tr></tbody></table></table-wrap><p>It is observed that for each case the dimension fractal, in the first place is not whole and it overcomes the three dimensions reaching the highest value the humidity, the same as the entropy that would indicate that it is the system with more disorder of the four that could be this values.</p></sec><sec id="s3_3"><title>3.3. Prediction of the Meteorological Variables</title><p><xref ref-type="table" rid="table8">Table 8</xref> Hypothesis test with distribution Z for half zero with significance level 0.01 to two lines (theoretical Z this among 2.58 and 2.58).</p></sec></sec><sec id="s4"><title>4. Conclusions</title><p> The studied systems are chaotic and hyperchaotic, according to the Theory of the Chaos (<xref ref-type="fig" rid="fig2">Figure 2</xref>) (they present positive bigger coefficients to one of Lyapunov), to exception of the precipitation in whose data correlation has not been determined in the used pattern.</p><p> The level of calculated (entropyvalue) chaoticity reaches higher values in the parameters of humidity, diminishing gradually respectively toward the pressure, temperature and speed of the wind.</p><p> The dimensions of the parameters are fractional that go diminishing from the humidity in the same order of the entropy (3.765), pressure (3.461), temperature (3.177) and speed of the wind (3.155) (<xref ref-type="table" rid="table2">Table 2</xref>).</p><p> Various atmospheric parameters with high correlation and low absolute deviations between predicted and actual data with the exception of the precipitation which shows no correlation can be predicted (Tables 3-7).</p><p> The data predicted generally tend to differ much more in time with respect to the real data (Figures 3-7 and Tables 3-7).</p><p> The data are statistically same, and given the results seen previously one can say that they have the same behavior whit the 99% of precision (<xref ref-type="table" rid="table8">Table 8</xref>).</p><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Comparison graph between real data and predictors of ambient temperature during 24 and 72 hours.</title></caption><fig id ="fig3_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x48.png"/></fig><fig id ="fig3_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x49.png"/></fig></fig-group><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Comparison graph between real data and predictors of humidity during 24 and 72 hours.</title></caption><fig id ="fig4_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x50.png"/></fig><fig id ="fig4_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x51.png"/></fig></fig-group><fig-group id="fig5"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Comparison graph between real data and predictors of speed of wind during 24 and 72 hours.</title></caption><fig id ="fig5_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x52.png"/></fig><fig id ="fig5_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x53.png"/></fig></fig-group><fig-group id="fig6"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Comparison graph between real data and predictors of pressure during 24 and 72 hours.</title></caption><fig id ="fig6_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x54.png"/></fig><fig id ="fig6_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x55.png"/></fig></fig-group><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Comparison graph between real data and precipitation predicted during 24 and 72 hours</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-4700296x56.png"/></fig><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> The fractal dimension and the entropy of each of the parameters values</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Fractal Dimension</th><th align="center" valign="middle" >Sistem Entropya</th></tr></thead><tr><td align="center" valign="middle" >Temperature</td><td align="center" valign="middle" >3.154834</td><td align="center" valign="middle" >0.004678229</td></tr><tr><td align="center" valign="middle" >Humidity</td><td align="center" valign="middle" >3.177086</td><td align="center" valign="middle" >0.010772463</td></tr><tr><td align="center" valign="middle" >Wind Speed</td><td align="center" valign="middle" >3.460514</td><td align="center" valign="middle" >0.015024107</td></tr><tr><td align="center" valign="middle" >Pressure</td><td align="center" valign="middle" >3.765306</td><td align="center" valign="middle" >0.034304828</td></tr><tr><td align="center" valign="middle" >Precipitation</td><td align="center" valign="middle" >---------------</td><td align="center" valign="middle" >----------------</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Correlation of the real data and prediction of temperature</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Pred 24</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Pred 72</th></tr></thead><tr><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Pred 24</td><td align="center" valign="middle" >0.90</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >Pred 72</td><td align="center" valign="middle" >0.93</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Correlation of the real data and predicted of humidity</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Pred 24</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Pred 72</th></tr></thead><tr><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Humedad</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Pred 24</td><td align="center" valign="middle" >0.88</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >Pred 72</td><td align="center" valign="middle" >0.82</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><table-wrap id="table5" ><label><xref ref-type="table" rid="table5">Table 5</xref></label><caption><title> Correlation of the real data and predicted of speed of the wind</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Pred 24</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Pred 72</th></tr></thead><tr><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Pred 24</td><td align="center" valign="middle" >0.91</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >Pred 72</td><td align="center" valign="middle" >0.83</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><table-wrap id="table6" ><label><xref ref-type="table" rid="table6">Table 6</xref></label><caption><title> Correlation of the real data and predicted of atmospheric pressure</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Predicha 24</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Predicha 72</th></tr></thead><tr><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Predicha 24</td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >Predicha 72</td><td align="center" valign="middle" >0.73</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><table-wrap id="table7" ><label><xref ref-type="table" rid="table7">Table 7</xref></label><caption><title> Correlation of the rainfall real and predicted data</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Prediction 24</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Real</th><th align="center" valign="middle" >Prediction 72</th></tr></thead><tr><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Real</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Prediction 24</td><td align="center" valign="middle" >−4.07E−18</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >Prediction 72</td><td align="center" valign="middle" >1.15E−16</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><table-wrap id="table8" ><label><xref ref-type="table" rid="table8">Table 8</xref></label><caption><title> Hypothesis test with distribution Z for half zero with significance level 0.01 to two lines (theoretical Z this among 2.58 and 2.58)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Parametro</th><th align="center" valign="middle" >Z</th></tr></thead><tr><td align="center" valign="middle" >Temperature</td><td align="center" valign="middle" >−0.27</td></tr><tr><td align="center" valign="middle" >Humidity</td><td align="center" valign="middle" >0.61</td></tr><tr><td align="center" valign="middle" >Wind Speed</td><td align="center" valign="middle" >−2.33</td></tr><tr><td align="center" valign="middle" >Pressure</td><td align="center" valign="middle" >2.14</td></tr><tr><td align="center" valign="middle" >Precipitation</td><td align="center" valign="middle" >−2.12</td></tr></tbody></table></table-wrap><p> It is a method that works properly despite the conditions of the city of Riobamba, by its geographical position and height with respect to the level of the sea, being able to recommend its use as an alternative to the traditional ones that do not work precisely in these conditions and hardly have access.</p></sec><sec id="s5"><title>Acknowledgements</title><p>Thanks to the alternative energy group of the ESPOCH for 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