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  <front>
    <journal-meta><journal-id journal-id-type="publisher">NPG</journal-id><journal-title-group>
    <journal-title>Nonlinear Processes in Geophysics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1607-7946</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/npg-26-291-2019</article-id><title-group><article-title>Mahalanobis distance-based recognition of changes<?xmltex \hack{\break}?> in the dynamics of a
seismic process</article-title><alt-title>Changes in the dynamics of a seismic process</alt-title>
      </title-group><?xmltex \runningtitle{Changes in the dynamics of a seismic process}?><?xmltex \runningauthor{T. Matcharashvili et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Matcharashvili</surname><given-names>Teimuraz</given-names></name>
          <email>matcharashvili@gtu.ge</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Czechowski</surname><given-names>Zbigniew</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhukova</surname><given-names>Natalia</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>M. Nodia Institute of Geophysics, Tbilisi State University, Tbilisi,
Georgia</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institute of Geophysics, Polish Academy of Sciences, Warsaw, Poland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Teimuraz Matcharashvili (matcharashvili@gtu.ge)</corresp></author-notes><pub-date><day>27</day><month>August</month><year>2019</year></pub-date>
      
      <volume>26</volume>
      <issue>3</issue>
      <fpage>291</fpage><lpage>305</lpage>
      <history>
        <date date-type="received"><day>23</day><month>December</month><year>2018</year></date>
           <date date-type="rev-request"><day>5</day><month>February</month><year>2019</year></date>
           <date date-type="rev-recd"><day>17</day><month>July</month><year>2019</year></date>
           <date date-type="accepted"><day>26</day><month>July</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 Teimuraz Matcharashvili et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019.html">This article is available from https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019.html</self-uri><self-uri xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e106">In the present work, we aim to analyse the regularity of
a seismic process based on its spatial, temporal, and energetic
characteristics. Increments of cumulative times, increments of cumulative
distances, and increments of cumulative seismic energies are calculated from
an earthquake catalogue for southern California from 1975 to 2017.</p>
    <p id="d1e109">As the method of analysis, we use the multivariate Mahalanobis distance
calculation, combined with a surrogate data testing procedure that is often
used for the testing of non-linear structures in complex data sets. Before
analysing the dynamical features of the seismic process, we tested the used
approach for two different 3-D models in which the dynamical features were
changed from more regular to more randomised conditions by adding a certain
degree of noise.</p>
    <p id="d1e112">An analysis of the variability in the extent of regularity of the seismic
process was carried out for different completeness magnitude thresholds.</p>
    <p id="d1e115">The results of our analysis show that in about a third of all the 50-data
windows the original seismic process was indistinguishable from a random
process based on its features of temporal, spatial, and energetic
variability. It was shown that prior to the occurrence of strong earthquakes,
mostly in periods of generation of relatively small earthquakes, the
percentage of windows in which the seismic process is indistinguishable from
a random process increases (to 60 %–80 %). During periods of aftershock
activity, the process of small earthquake generation became regular in all
of the windows considered, and thus was markedly different from the
randomised catalogues.</p>
    <p id="d1e118">In some periods within the catalogue, the seismic process appeared to be
closer to randomness, while in other cases it became closer to a regular behaviour. More specifically, in periods of relatively
decreased earthquake generation activity (with low energy release), the
seismic process appears to be random, while during periods of occurrence of
strong events, followed by series of aftershocks, significant deviation from
randomness is shown, i.e. the extent of regularity markedly increases. The
period for which such deviation from random behaviour lasts depends on the
amount of seismic energy released by the strong earthquake.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e130">The process of earthquake generation remains a focus of diverse
interdisciplinary investigations by Earth science researchers worldwide. The
practical and scientific reasons for this interest are well known and easily
explainable. However, despite this strong interest and the enormous research
efforts that have already been applied, many important aspects of the
complex seismic process characterised by space and time clustering are still
not clear (Bowman and Sammis, 2004; Godano and Tramelli, 2016; Kossobokov
and Nekrasova, 2017; Matcharashvili et al., 2018; Pasten et al., 2018).</p>
      <p id="d1e133">One of the fundamental questions of modern Earth science concerns the
dynamics of the seismic process. As a logical compromise between the
different approaches that have been proposed for this problem, it has been
suggested that the dynamical features of the seismic process may vary,
ranging from periodic (primarily for large events) to the totally random
occurrence of earthquakes (Matcharashvili et al., 2000; Corral, 2004;
Davidsen and Goltz, 2004). The same, in terms of the concept of intermittent
criticality of earthquake generation, can be expressed as the ability of a
tectonic system to<?pagebreak page292?> approach and/or retreat from the critical state, i.e. the
state of the system in which strong earthquakes occur (see e.g. Sornette
and Sammis, 1995; Bowman et al., 1998; Bowman and Sammis, 2004; Corral,
2004).</p>
      <p id="d1e136">Current knowledge of the scaling and memory characteristics of the overall
seismic process indeed supports this proposed diversity in the dynamics of
earthquake generation (Sornette and Sammis, 1995; Bowman et al., 1998;
Abe und Suzuki, 2004; Chelidze and Matcharashvili, 2007; Czechowski, 2001, 2003;
Białecki and Czechowski, 2010; Kossobokov and Nekrasova, 2017). Moreover,
the results of analyses carried out to assess the dynamical features of the
seismic process in terms of its separate domains (time, space, and energy)
also indicate differences in behaviour (see e.g. Goltz, 1998; Matcharashvili
et al., 2000, 2002; Abe and Suzuki, 2004; Chelidze and Matcharashvili,
2007; Iliopoulos et al., 2012). More specifically, it has been shown that
the seismic process in the temporal and spatial domains may reveal features
that are close to so-called low-dimensional dynamical structures, although
the features of the behaviour in the energy domain appear close to
randomness, i.e. representing high-dimensional dynamical processes (Goltz,
1998; Matcharashvili et al., 2000; Iliopoulos et al., 2012). This has been
shown for whole catalogues as well as for their parts and for different
time periods.</p>
      <p id="d1e139">Coming back to the concept of a critical state, it should be emphasised that
intermittent criticality implies time-dependent variations in the activity
during a seismic cycle. Thus, since the critical state is usually described
as the state of the system when it is at the boundary between order and
disorder (Bowman et al., 1998), we can describe the time variability of the
seismic process in terms of the contemporary concept of geocomplexity
(Rundle et al., 2000).</p>
      <p id="d1e143">According to present knowledge, and in complete accordance with the concept
of intermittent criticality, it is accepted that the extent of regularity
(order) of the seismic process may vary in all its domains (temporal,
spatial, and energetic) (Goltz, 1998; Abe and Suzuki, 2004; Chelidze and
Matcharashvili, 2007; Iliopoulos et al., 2012; Matcharashvili et al., 2000,
2002, 2018). At the same time, despite the large number of recent
publications demonstrating the diversity of these changes in the dynamics of
the seismic process, interest in this issue continues to grow. In this
context, it should be emphasised that it is important to assess these
dynamical changes on the basis of multivariate analysis, taking into account
all the temporal, spatial, and energetic constituents of the seismic process.
Thus, one important research task is to understand the character of these
changes in the entire seismic process.</p>
      <p id="d1e146">Based on the state-of-the-art studies mentioned above, we aim in the present
work to investigate the dynamical features of the seismic process based on
all its temporal, spatial, and energetic characteristics. We carry out a
multivariate comparison of the seismic process using an original earthquake
catalogue for southern California and a set of randomised catalogues in
which unique (temporal, spatial, and energetic) dynamical structures have
been intentionally distorted by a shuffling procedure. This
multivariate comparison of an original catalogue with randomised catalogues
may help us to gain new knowledge about the character of the changes that
occur in the extent of order/disorder of the seismic process. In
addition, we will have stronger arguments regarding where and how the
dynamics of the original seismic process in the analysed catalogue was close
to disorder (irregularity) or order (regularity). We also aim to determine
whether such changes are related to the process of preparation for strong
earthquakes.</p>
      <p id="d1e149">The results obtained in our research show that the extent of regularity in
the analysed seismic process changes and is closer to randomness
in the periods prior to strong earthquakes. After strong earthquakes, the
regularity of the original seismic process assessed based on its temporal,
spatial, and energetic characteristics is clearly increased.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data used</title>
      <p id="d1e160">We based our analysis on the southern California (SC) earthquake catalogue,
which is available from <uri>http://www.isc.ac.uk/iscbulletin/search/catalogue/</uri> (last access: November 2018). We focused on the
time period from 1975 to 2017 (see Fig. 1). According to results of a time
completeness analysis, the SC earthquake catalogue for the considered period
is complete for <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.6</mml:mn></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e180">Map of the area covered by the southern California earthquake catalogue
(1975–2017).</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f01.png"/>

      </fig>

      <p id="d1e189">As pointed out above, we aimed to carry out a multivariate analysis of the
dynamical features of the seismic process. Thus, in order to preserve the
original character of the temporal, spatial, and energetic characteristics of
this process, we intentionally avoided any cleaning or filtering of<?pagebreak page293?> the
earthquake catalogue used here. This approach was based on a widely accepted
practice (see e.g. Bak et al., 2002; Christensen et al., 2002; Corral, 2004;
Davidsen and Goltz, 2004; Matcharashvili et al., 2018) in which all events
are assumed to be on the same footing and the catalogue is considered as a
whole. In other words, we did not pay attention to the details of tectonic
features, the locations of the earthquakes, or their classification as
mainshock or aftershock (Bak et al., 2002; Christensen et al., 2002; Corral,
2004).</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Methods of analysis</title>
      <p id="d1e200">In view of our research goal, i.e. a multivariate assessment of the extent
of the regularity of the original seismic process, we need to analyse the
seismic process in terms of the simultaneous variability in all three of
its domains: temporal, spatial, and energetic. From this point of view, we
consider cumulative sums of the characteristics of earthquakes in the
temporal, spatial, and energetic domains (Fig. 2). The cumulative sum
representation in the time domain is trivial, since time is already a
cumulative characteristic, representing the cumulative sum of
inter-earthquake times. Cumulative representation in the spatial domain is
also quite feasible, and we consider cumulative sums of distances between
consecutive earthquakes in the seismic catalogue. The cumulative sum of
seismic energies released by consecutive earthquakes is also often used in
the context of the different aspects of earthquake generation (e.g. Bowman et al, 1998; Bowman and Sammis, 2004; Nakamichi et al., 2018). Here, we add that despite some
controversies (see e.g. Corral, 2004, 2008) over the question of the
reliable energetic measurement of earthquake size, its relation to the
magnitude of an earthquake is generally accepted. Thus, from the earthquake
magnitudes in the SC catalogue, we can calculate the amount of seismic
energy released, according to Kanamori (1977).</p>
      <p id="d1e203">We start from the first earthquake in the catalogue (for the time period of
interest, from 1975 to 2017), which we consider a starting point, and
then follow the time sequence. Thus, ICT(<inline-formula><mml:math id="M2" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) is the <inline-formula><mml:math id="M3" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>th interevent time (i.e. the
time between the <inline-formula><mml:math id="M4" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>th earthquake and the (<inline-formula><mml:math id="M5" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>-1)th earthquake); ICD(<inline-formula><mml:math id="M6" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) is the distance
between consecutive events and ICE(<inline-formula><mml:math id="M7" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) is the energy of the <inline-formula><mml:math id="M8" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>th earthquake. We can
also define these quantities in terms of increments of the cumulative sums;
i.e. ICT(<inline-formula><mml:math id="M9" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M10" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M11" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) are the increments of cumulative sums of the interevent times,
interevent distances, and seismic energy released by consecutive earthquakes,
respectively.</p>
      <p id="d1e277">In order to have the same standard deviation for the three groups of data,
the standard deviations were calculated for each of the ICT(<inline-formula><mml:math id="M12" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M13" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M14" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) data sets, and the
data sets were then normalised to have their standard deviations equal to 1.</p>
      <p id="d1e301">In order to characterise the seismic process from a multivariate point of
view, we used a well-known statistical test, the Mahalanobis distance (MD)
calculation. Calculation of the MD is an effective multivariate method for
different classification purposes and is often used for data sets of
different origins. Thus, the objective of our analysis can be regarded as a
classification task of the features of a seismic process, assessed using the
variability in ICT(<inline-formula><mml:math id="M15" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M16" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M17" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e328">Cumulative sums of <bold>(a)</bold> interevent times; <bold>(b)</bold> inter-earthquake
distances; and <bold>(c)</bold> released seismic energies, starting from the first event
in the southern California catalogue (1975–2017).</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f02.png"/>

      </fig>

      <p id="d1e346">In other words, we aimed to assess the changes that occurred in the seismic
process over the period covered by the SC catalogue (1975–2017). It is
well known that the correctness of a multivariate assessment and
classification of a system is strongly dependent on correct feature
extraction (McLachlan, 1992, 1999). In other words, the data sets
used should be specifically focused on the targeted features of the process
under investigation. Hence, in order to have data sets with a similar
physical sense, enabling us to assess the dynamical features of seismicity
in three domains, we used ICT(<inline-formula><mml:math id="M18" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M19" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M20" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) data sets.</p>
      <?pagebreak page294?><p id="d1e370">The MD (Mahalanobis, 1930; McLachlan, 1992, 1999) is a widely accepted
method of measuring the separation of two groups of vectors (e.g. one group
A, consisting of <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> vectors <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), and
another group B, with <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> vectors <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). In this method, the difference
between the groups can be considered in terms of the difference between the
mean vectors <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo></mml:mrow></mml:math></inline-formula> of each group relative to the common within-group
variation. This allows us to draw a conclusion on whether the investigated
groups are similar or dissimilar. The MD (often denoted as <inline-formula><mml:math id="M27" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>) can be
calculated from the following expression:
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M28" display="block"><mml:mrow><mml:msup><mml:mi>D</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mfenced close="〉" open="〈"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>-</mml:mo><mml:mfenced open="〈" close="〉"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:msup><mml:mi/><mml:mi mathvariant="normal">T</mml:mi></mml:msup><mml:msup><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mfenced close=")" open="("><mml:mrow><mml:mfenced close="〉" open="〈"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>-</mml:mo><mml:mfenced open="〈" close="〉"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="bold">S</mml:mi></mml:math></inline-formula> is the pooled covariance matrix
          <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M30" display="block"><mml:mrow><mml:mi mathvariant="bold">S</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        and <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are covariance matrices of the corresponding groups,
e.g.
          <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M33" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msubsup><mml:mi mathvariant="bold">X</mml:mi><mml:mi mathvariant="normal">A</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msubsup><mml:msub><mml:mi mathvariant="bold">X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        The superscripts “T” and “<inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>” denote the transpose and the inverse operators,
respectively. The rows of matrix <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">X</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) form the components of the
<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) vectors <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, e.g.
          <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M40" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold">X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced close="]" open="["><mml:mtable class="array" columnalign="center center center"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi>x</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi>z</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mi mathvariant="normal">…</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi mathvariant="normal">…</mml:mi></mml:mtd></mml:mtr></mml:mtable></mml:mtd><mml:mtd><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mi mathvariant="normal">…</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi mathvariant="normal">…</mml:mi></mml:mtd></mml:mtr></mml:mtable></mml:mtd><mml:mtd><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mi mathvariant="normal">…</mml:mi></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi mathvariant="normal">…</mml:mi></mml:mtd></mml:mtr></mml:mtable></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mi>x</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mi>z</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        In general, two conditions or states of a system are more likely to fall
into the same class or group (or have a higher probability of being similar)
if the calculated MD value is smaller. In order to assess the significance
of the difference between the groups, Hotelling's <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msup><mml:mi>T</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> statistic was
used, converted into an <inline-formula><mml:math id="M42" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> value and assessed using an <inline-formula><mml:math id="M43" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> test. The <inline-formula><mml:math id="M44" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> value was
calculated as follows:
          <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M45" display="block"><mml:mrow><mml:mi>F</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>p</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">B</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi>D</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        In Eq. (5),   <inline-formula><mml:math id="M46" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>   is     the degrees of freedom. Then, in order to draw a final conclusion on the similarity or dissimilarity of the two groups, we compare the calculated   <inline-formula><mml:math id="M47" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> values with a critical value   <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (corresponding to the degrees of freedom). In the case where   <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mi>F</mml:mi><mml:mo>&gt;</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, a statistically significant difference between the groups is established,  with a specific probability (significance level).</p>
      <p id="d1e1050">When dealing with analysis of complex seismic processes, it needs to be
pointed out that the MD calculation is sensitive to inter-variable changes
in a multivariate system (Mahalanobis, 1930; Lattin et al., 2003) and that
it takes into account the correlations between several variables providing
information on the similarity or dissimilarity between the compared groups
(Taguchi and Jugulum, 2002; Kumar et al., 2012).</p>
      <p id="d1e1053">If we are primarily interested in analysing dynamical changes occurring on
short scales (short data sets), it is useful to combine the advantages of
multivariate analysis and surrogate testing (Matcharashvili et al., 2017, 2018). In
this case, we can use the multivariate MD calculation to examine whether the
original seismic process is similar to or dissimilar from a random process
(randomised catalogues) by comparing them based on the three main
characteristics listed above.</p>
      <p id="d1e1056">In summary, we aim to analyse the way in which the order in the seismic
process, as assessed using its derivative temporal, spatial, and energetic
characteristics (the quantities ICT(<inline-formula><mml:math id="M50" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M51" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M52" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>)), changes over the period of analysis.
To achieve this, we compare the original SC earthquake catalogue
(1975–2017) with a set of artificial catalogues in which the original
dynamical structures (of the temporal, spatial, and energetic distributions)
have been intentionally destroyed by a shuffling procedure (Kantz and
Schreiber, 1998). We generated 100 such randomised catalogues. In order to
analyse the seismic process, we divided these catalogues into consecutive,
non-overlapping 50-data windows shifted by 50 data. Thus, each window from
the original catalogue represents group A, and each window from the shuffled
catalogue forms a group B (we have a total of 100 B groups). For example,
the vector <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mtext>ICT</mml:mtext><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mtext>ICD</mml:mtext><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mtext>ICE</mml:mtext><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Testing the method on models</title>
      <p id="d1e1169">In order to verify whether the approach used here, which combines MD
calculation with surrogate testing, is indeed useful for discerning any changes
occurring in the natural 3-D system (the seismic process in a tectonic
system), with slightly or strongly different dynamical features, we used
time series generated by two 3-D simulated systems with added noise. These
were a 3-D Lorenz system and a crack fusion model with added Gaussian noise.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Lorenz model</title>
      <p id="d1e1179">The well-known Lorenz model describes the motion of an
incompressible fluid contained in a cell that has a higher temperature at
the bottom and a lower temperature at the top. Despite the simple form of
this set of equations, very complex behaviour can be exhibited. This approach
has therefore been commonly used to present the interesting non-linear
dynamics of 3-D systems.</p>
      <p id="d1e1182">The Lorenz model has the following form (see e.g. Hilborn, 1994):
            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M54" display="block"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi>p</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi>x</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi>x</mml:mi><mml:mi>z</mml:mi><mml:mo>+</mml:mo><mml:mi>r</mml:mi><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>z</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi>x</mml:mi><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi>b</mml:mi><mml:mi>z</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          where <inline-formula><mml:math id="M55" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> represents the Prandtl number, <inline-formula><mml:math id="M56" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> is the Rayleigh number, and <inline-formula><mml:math id="M57" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> is
related to the ratio of the vertical height of the fluid layer to the
horizontal size of the convection rolls. For values of <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>,
trajectories in 3-D space (<inline-formula><mml:math id="M59" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M60" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M61" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>) are attracted by the origin (0, 0, 0). When
<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, the Lorenz model has three fixed points which can have
different features.</p>
      <?pagebreak page295?><p id="d1e1353">In this work, we need time series that are close to stationary, and thus in
order to avoid periodic orbits we assume <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, namely <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula>. In
order to generate our time series, we use the discrete version of the Lorenz
equations that are modified by the introduction of two random noise terms:
            <disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M65" display="block"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>p</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>c</mml:mi><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>r</mml:mi><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>c</mml:mi><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>b</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>c</mml:mi><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          The first noise term, <inline-formula><mml:math id="M66" display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula>, is the same (i.e. has the same value) in all
three equations and for all cases under investigation. Due to fluctuations
generated by the noise, the states of the system are around the attractor at
the origin (0, 0, 0). The Lorenz model with only the <inline-formula><mml:math id="M67" display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> noise term will
be treated as a basic reference system, i.e. a “deterministic” system. The
second noise term <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is
generated separately for each of the three equations. It is multiplied by
the parameter <inline-formula><mml:math id="M71" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> whose values will increase. The role of the
second noise term is to check the influence of increasing randomness on the
measures of order in the process. To generate time series using the system
in Eq. (5), we assume the following values for the parameters: <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi>c</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula>. The initial values are (<inline-formula><mml:math id="M76" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>(0), <inline-formula><mml:math id="M77" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>(0), <inline-formula><mml:math id="M78" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>(0)) <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">20</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the time step is <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula>. The parameter <inline-formula><mml:math id="M81" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> increases
from 0.0 (for the reference system) to 1.0.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Crack fusion model</title>
      <p id="d1e1788">The kinetic crack fusion model (Czechowski,
1991, 1993, 1995) describes the evolution of a system of numerous cracks
which can nucleate, propagate, and coalesce under applied stress. Here, we
use a simple version of the model (related to seismic processes) in which
only three crack populations (small cracks <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, medium cracks <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and large
cracks <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are taken into account. Their evolution is governed by the
following system of non-linear equations:
            <disp-formula id="Ch1.E8" content-type="numbered"><label>8</label><mml:math id="M85" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{9}{9}\selectfont$\displaystyle}?><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi>x</mml:mi><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mi>x</mml:mi><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mi>x</mml:mi><mml:mi>z</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mi>z</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>T</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi>x</mml:mi><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi>y</mml:mi><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi>x</mml:mi><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mi>y</mml:mi><mml:mi>z</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>z</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi>x</mml:mi><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:mi>y</mml:mi><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mi>a</mml:mi><mml:mi>z</mml:mi><mml:mi>z</mml:mi><mml:mo>-</mml:mo><mml:mi>g</mml:mi><mml:mi>z</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
          where the parameters <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are related to the probability of
coalescence, <inline-formula><mml:math id="M88" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> is the nucleation rate of small cracks around large cracks,
and <inline-formula><mml:math id="M89" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> is the healing rate of large cracks. The second source term for small
cracks is due to the external stress <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,  which can grow in response to
relative tectonic plate motion and diminish according to the number of large
cracks <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, i.e.
            <disp-formula id="Ch1.E9" content-type="numbered"><label>9</label><mml:math id="M92" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>v</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi>T</mml:mi><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0</mml:mn></mml:mtd><mml:mtd><mml:mrow><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>
          In a similar way to the Lorenz model, the crack fusion model exhibits two
kinds of behaviour: it can decay to one stationary point or its attractor
can be given by periodic orbits. As above, we need stationary-like time
series, so in order to avoid periodic orbits, we assume the parameters
<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mo>&lt;</mml:mo><mml:mo>(</mml:mo><mml:mi>v</mml:mi><mml:mi mathvariant="italic">μ</mml:mi><mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">crit</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6320</mml:mn></mml:mrow></mml:math></inline-formula> and modify the
hierarchical system by introducing two random noise terms <inline-formula><mml:math id="M94" display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to the equation for small cracks only.
            <disp-formula id="Ch1.E10" content-type="numbered"><label>10</label><mml:math id="M96" display="block"><mml:mtable rowspacing="0.2ex" class="split" columnspacing="1em" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>c</mml:mi><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:msub><mml:mi mathvariant="italic">ζ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>(</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mfenced open="(" close=""><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced close=")" open=""><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mi>a</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>g</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>z</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          In order to generate time series using the system of equations in Eq. (10), we
assume the following values for the parameters: <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mi>c</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.45</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula>, initial
values (<inline-formula><mml:math id="M105" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>(0), <inline-formula><mml:math id="M106" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>(0), <inline-formula><mml:math id="M107" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>(0)) <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">20</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and time step <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. The
parameter <inline-formula><mml:math id="M110" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> increases from 0.0 (for the reference system) to
0.35.</p>
      <p id="d1e2856">Thus, in order to ensure that the multivariate method used here enables us
to discriminate between different conditions of dynamical systems, we use 3-D
models in which the dynamical features are changed from more regular to more
randomised conditions by adding some extent of noises. We start with the
Lorenz system (Fig. 3) and then proceed to the crack fusion model
(Czechowski, 1991, 1993, 1995) (Fig. 4). As explained above, in both cases
we add noises of different intensity to the original 3-D system, assuming that
the more intense the added noise, the closer the model system is to
randomness. Figures 3 and 4 clearly show that the number (or portion) of the
50-data windows in which the condition of the 3-D system is indistinguishable
from the initial condition (the system with no added noise) gradually
decreases when the intensity of the added noise is increased. This means
that the method of analysis used here enables us to distinguish the
conditions of systems even in cases when they are only slightly different
(i.e. only a small amount of noise is added) (see the left-hand parts of the
curves in Figs. 3 and 4, showing a smaller amount of added noise).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e2861">Percentage of the 50-data windows (shifted by 50 data steps) of the
Lorenz system with added noise that are indistinguishable from the initial
condition (system with no added noise).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e2873">The percentage of the 50-data windows (shifted by 50 data steps) of
the crack fusion model with added noise that are indistinguishable from the
initial condition (system with no added noise).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f04.png"/>

        </fig>

      <?pagebreak page296?><p id="d1e2882">For clarity, we note here that in Figs. 3 and 4, we show results for the
case of windows 50-data long, since in the analysis of the seismic catalogue
below, we also use this size of window. At the same time, it should be
emphasised that the result of the above analysis depends on the timescale
used (the size of the windows). For larger windows (500- or 1000-data long,
for example) distinguishability from the starting condition (i.e. without
added noise) requires a larger amount of added noise, although the general
conclusion remains the same: the method of analysis used here enables us to
distinguish between the states of 3-D systems with different extents (or
degrees) of dynamical regularity.
<?xmltex \hack{\newpage}?></p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Results and discussion</title>
      <p id="d1e2896">Having shown that the multivariate testing method selected for this research
enables us to discriminate between different conditions of dynamical
systems, we proceed to analyse data sets from the original seismic catalogue and the randomised catalogues mentioned above. We start
from the case where MD values are calculated for non-overlapping, 50-data,
windows shifted by 50 data steps, in the same way as for the 3-D model data
sets. Figure 5 presents the results of this calculation. Groups consisting of
the ICT(<inline-formula><mml:math id="M111" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M112" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M113" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) columns from the original catalogue were compared with the
corresponding three columns of ICT(<inline-formula><mml:math id="M114" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M115" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M116" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) data from each of 100 randomised catalogues
(shuffled in time, space, and by magnitudes). In this way, the MD(<inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values
were calculated. The MD values shown in Fig. 5 are averages of the MD(<inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
values calculated for each of the randomised catalogues. The dashed lines in
this figure and the following figures indicate the critical value <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which
was discussed in the previous section. For the number of degrees of freedom
used in this research, <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.99</mml:mn></mml:mrow></mml:math></inline-formula>, corresponding to a significant difference
between the groups with <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula> (MD <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.68</mml:mn></mml:mrow></mml:math></inline-formula> corresponds to <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.99</mml:mn></mml:mrow></mml:math></inline-formula>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e3028">Seismic energy released (upper curve) and average MD values (bottom
curve) calculated for consecutive non-overlapping 50-data windows shifted
by 50 data steps, for the southern California earthquake catalogue
(1975–2017). Averages of the MD values and the corresponding standard
deviations (given in the lower plot by white circles and grey error bars)
were calculated by comparing ICT(<inline-formula><mml:math id="M124" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M125" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M126" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences in the
original catalogue and in the set of randomised catalogues. The dotted line
corresponds to a significant difference between windows at <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f05.png"/>

      </fig>

      <p id="d1e3070">For a more precise analysis, we calculate the MD values for 50 data windows
shifted by one data step (Fig. 6).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e3076">Average MD values calculated by comparing ICT(<inline-formula><mml:math id="M128" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M129" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M130" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences from the
original SC catalogue and from the set of randomised catalogues. The dotted
line corresponds to a significant difference between windows at <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. MD
values are calculated for 50 data windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f06.png"/>

      </fig>

      <p id="d1e3118">The results in Figs. 5 and 6 support the view that despite the generality of
the background physics (Lombardi and Marzocchi, 2007; Di Toro et al., 2004;
Davidsen and Goltz, 2004; Helmstetter, 2003;  Helmstetter and Sornette, 2002;  Corral, 2008),
the processes taking place prior to and after main shocks are nevertheless
different (Sornette and Knopoff, 1997; Davidsen and Goltz, 2004; Wang and
Kuo, 1998). According to recent research, the latter is characterised by
long- and short-range correlations and thus is more ordered, while the
former is apparently more uncorrelated and random-like (Touati et al., 2009;
Godano, 2015). Indeed, according to Bowman et al. (1998), the loss of energy
(released also in the form of seismic energy) that is related to the
occurrence of strong events introduces memory into the system (Bowman and
Sammis, 2004).</p>
      <p id="d1e3121">We can see from Figs. 5 and 6 that in the SC earthquake catalogue considered
here, the seismic process after strong earthquakes is more regular than in
the periods prior to these<?pagebreak page297?> events. Indeed, in all windows, the seismic
process, as assessed based on the variability  in  ICT(<inline-formula><mml:math id="M132" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M133" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M134" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), after strong
earthquakes is significantly different from the randomised catalogues. In
contrast, the majority of the 50-data windows examined here show that the
original seismic process prior to strong earthquakes is statistically
indistinguishable from the randomised catalogues (see Figs. 5 and 6). It is
important to mention that the windows, located prior to strong earthquakes,
make up 33 % of the total number of windows in the entire catalogue.
Moreover, if we consider only those periods in the catalogue that
immediately precede strong earthquakes, the proportion of windows in which
the seismic process is indistinguishable from randomness increases to
60 %–80 %. Thus, in the overwhelming majority of windows that
immediately precede strong earthquakes, the seismic process is
indistinguishable from that observed in the randomised catalogues. The
seismic process in these parts of the original catalogue can therefore be
regarded as random-like.</p>
      <p id="d1e3145">In order to exclude the possibility that some of the characteristics
selected here (ICT(<inline-formula><mml:math id="M135" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M136" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M137" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>)) may have more influence on the results than the
others, we carried out a similar analysis comparing groups of original and
randomised catalogues by two of the three characteristics. The results of
this separate comparison of the groups, using pairs of columns  (ICT(<inline-formula><mml:math id="M138" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) and ICD(<inline-formula><mml:math id="M139" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>); ICT(<inline-formula><mml:math id="M140" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) and  ICE(<inline-formula><mml:math id="M141" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>); ICD(<inline-formula><mml:math id="M142" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) and
ICE(<inline-formula><mml:math id="M143" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>)), are not shown here, but generally coincide with the results of the above
analysis (using all three columns). This indicates that the results of our
analysis cannot be reduced to the influence of only a single characteristic.
Thus, the changes shown in Figs. 5 and 6 reveal changes in the dynamical
features of the seismic process as whole, involving changes in all three of
its domains.</p>
      <p id="d1e3212">For better visualisation of the above results (see Fig. 6), Fig. 7 presents
MD values calculated for 50 data windows for the period from 14 May 1990 (the
window started from event 12100 in the SC catalogue) to 28 June 1992 (the
window started from event 13797 in the SC catalogue). Within this period,
two strong earthquakes occurred, <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula> (23 April 1992) and <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula> (28 June 1992).
Prior to both of these strong earthquakes, we observe windows in which the
seismic process is indistinguishable from the randomised catalogues in terms
of the variation in  ICT(<inline-formula><mml:math id="M146" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M147" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M148" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) data (see circles below the dotted significant
difference line). It is also noticeable that after these strong events, the
extent of order in the seismic process strongly increases, as shown by the
changes in MD values (the original catalogue becomes more different from the
randomised catalogue). For <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula>, unlike the <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula> event, this increase lasted
for a considerable time after the strong event, at least until January 1993
(see Fig. 6).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e3284">Average MD values calculated for the period from 14 May 1990 (12100)
to 28 June 1992 (13797) in which two strong earthquakes occurred: <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula>
(23 April 1992) and <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula> (28 June 1992). MD values are calculated by comparing
ICT(<inline-formula><mml:math id="M153" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M154" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M155" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences from the original SC catalogue and from the set of
randomised catalogues. The dotted line corresponds to a significant
difference between windows at <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. MD values are calculated for 50-data
windows shifted by one data step.
</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f07.png"/>

      </fig>

      <p id="d1e3349">The next period selected for detailed analysis was from 24 August 1997 (the window
started from event 20760 in the SC catalogue) to 16 October 1999 (the window
started from event 21160 in the SC catalogue). Two large events occurred in
this period: a moderate <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">5.23</mml:mn></mml:mrow></mml:math></inline-formula> earthquake (6 March 1998) and a strong <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula>
earthquake (16 October 1999). Here, we note the obvious fact that there is no use
trying to find the magnitude range that may occur in windows where
seismicity behaves in a random-like way. Indeed, our results show (see Figs. 5, 6, and 7) that earthquakes of any size may occur in any window, both those
in which the seismic process is closer to regular behaviour and where it is
more random. Hence, we cannot speak about a magnitude threshold or about a
range of magnitudes in the sense of their immediate influence on changes in
the extent of the regularity of seismic process. On the other hand, our
results show that during periods of mostly small earthquake generation,
prior to the occurrence of a strong earthquake, the seismic process in the
majority of windows is indistinguishable from randomness. Thus, as assessed
based on simultaneous variations in ICT(<inline-formula><mml:math id="M159" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M160" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M161" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), the seismic process of relatively
small earthquakes' generation prior to strong earthquakes can be regarded as
being random-like.</p>
      <?pagebreak page298?><p id="d1e3395">The results shown in Fig. 8 are mostly similar to those in Fig. 7. Strong
and relatively strong (for this selected short period) earthquakes are
preceded by a significant number of windows in which the seismic process in
the original catalogue is indistinguishable from that observed for
randomised catalogues. In contrast, in all 50-data windows following strong
(or relatively strong) earthquakes, we can observe a statistically
significant difference. A multivariate comparison of these windows based on
the variation in ICT(<inline-formula><mml:math id="M162" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M163" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M164" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) demonstrates that in these windows, the original
seismic process is significantly different from the processes taking place
in the randomised catalogues (see Figs. 7 and 8).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e3421">Average MD values calculated for the period from 24 August 1997 (20760) to
16 October 1999 (21160) in which two strong earthquakes occurred: <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">5.23</mml:mn></mml:mrow></mml:math></inline-formula>
(6 March 1998) and <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula> (16 October 1999). The MDs are calculated by comparing
ICT(<inline-formula><mml:math id="M167" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M168" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M169" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences from the original SC catalogue and from the set of
randomised catalogues. The dotted line corresponds to a significant
difference between the windows at <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. MD values are calculated for 50-data windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f08.png"/>

      </fig>

      <p id="d1e3486">Separate consideration of the period of the strong <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula> earthquake
occurrence leads to a similar conclusion. From Fig. 9, we can again observe
that prior to strong earthquakes, the seismic process looks mostly random,
and that the extent of order strongly increases after these events.</p>
      <p id="d1e3501">As expected, the behaviour of the seismic process prior to and following all
of the strong events considered here is similar. The only difference is the
length of the period during which the post-earthquake seismic process
remains significantly regular compared to the randomised catalogues. For
strong earthquakes, this period is clearly longer (see Fig. 6). This appears
to be connected with the generation of a series of aftershocks, in which the
spatial, temporal, and energetic features are causally related to the
mainshock. This is in agreement with the well-known productivity law that
states that the larger the magnitude of the mainshock, the larger the total
number of aftershocks (Helmstetter, 2003; Baiesi and Paczuski, 2004; Godano
and Tramelli, 2016). Here, we emphasise that the question of the temporal
length of the aftershock sequence following a strong earthquake is still not
understood, as it is related to the timescale of background seismic activity
(Godano and Tramelli, 2016).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e3506">Average MD values calculated for the period from 30 October 2008 (27300)
to 5 April 2010 (28300) in which three moderate and strong earthquakes
occurred: <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">5.0</mml:mn></mml:mrow></mml:math></inline-formula> (1 October 2009), <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">5.8</mml:mn></mml:mrow></mml:math></inline-formula> (30 December 2009), and <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula> (4 April 2010). MDs
are calculated by comparing ICT(<inline-formula><mml:math id="M175" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M176" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M177" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences from the original SC catalogue
and from the set of randomised catalogues. The dotted line corresponds to a
significant difference between windows at <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. MD values are calculated
for 50-data windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f09.png"/>

      </fig>

      <p id="d1e3582">From Figs. 7 to 9, we can see that the extent of order in the seismic
process (as assessed based on the temporal, spatial, and energetic
distributions of earthquakes) may change not only in the periods prior to
and following strong (<inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula>) earthquakes, but also prior to
and following other events that are not as strong, or even moderate.
For example, as can be seen from Fig. 8, the <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.93</mml:mn></mml:mrow></mml:math></inline-formula> (14 May 1999, in
window 21570) and <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.71</mml:mn></mml:mrow></mml:math></inline-formula> (24 August 1999, in window 21776) earthquakes are
preceded by windows in which the seismic process mostly appears random, and
are followed by windows in which the extent of order of the seismic process
is markedly increased. The only difference is that for strong earthquakes,
the number of windows in which the extent of order increases is much larger
than for moderate ones. A similar conclusion can be drawn from Figs. 7 and
9. Thus, the most important conclusion is that prior to almost all strong
earthquakes, in periods which can be regarded as relatively seismically
calm, the original seismic process is indistinguishable from a random
process, as assessed based on the MD values calculated for windows of 50-data sequences of ICT(<inline-formula><mml:math id="M184" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M185" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M186" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) characteristics. In this sense, the end part of the
catalogue analysed in our work (where we found a long sequence of windows
(see Figs. 5 and 6) in which the seismic process is indistinguishable from
randomness, observed in a period when seismic activity could be regarded as
relatively calm) is particularly interesting regarding the future activity
of the fault.<fn id="Ch1.Footn1"><p id="d1e3662">Here we point out that this article was submitted to <italic>NPG</italic> at the end of 2018. Further development when in July 2019, two strong earthquakes <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">6.4</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula> occurred in the considered catalogue area, additionally convinced us that random-like behaviour of seismic processes may indeed be regarded as one of possible precursory markers of strong earthquakes.</p></fn></p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e3692">Magnitudes and MD values calculated for part of the SC catalogue
after <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula> (28 June 1992, sequential number in SC catalogue 13648) from
1 July 1992 (sequential number in SC catalogue 14608) to 5 July 1992
(sequential number in SC catalogue 15280). Average MD values are
calculated for 50-data windows shifted by one data step; 90 % of the
earthquakes in this period occurred within a distance of 0.5–70 km from the
epicentre of <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f10.png"/>

      </fig>

      <?pagebreak page299?><p id="d1e3723">Since the above results suggest that, prior to strong earthquakes, a
comparatively calm seismic process of relatively small (with <inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>,
Hough and Jones, 1997) earthquake generation is random-like, it was necessary to
carry out an additional analysis of the behaviour of these small events in
the case where they occur in windows after strong events. To achieve this,
we selected periods of relatively low seismic activity, involving events
with magnitudes <inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>. We considered 2- to 5-day periods of
aftershock activity that was weaker than <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula> (soon after strong
earthquakes). Figures 10 to 12 show the results of analysis for three such
periods following strong earthquakes of <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula>. As can be seen
from these figures, there are no windows in which the original seismic
process, according to MD values calculated for windows of ICT(<inline-formula><mml:math id="M197" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M198" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and
ICE(<inline-formula><mml:math id="M199" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) characteristics, can be regarded as random-like. In all of the windows
analysed, when a clear aftershock activity follows immediately after a
strong earthquake, the seismic process is significantly different from a
random process. In other words, in the original catalogue, the seismic
process after strong events in periods of relatively small (<inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>)
earthquake generation is significantly more regular than the randomised
catalogues. It can also be noted that a similar situation was seen for
sequences of small events occurring after other strong earthquakes in the
analysed catalogue. This offers further evidence that in periods of
aftershock activity, the original seismic process is strongly different from
that observed for the randomised catalogues in which we distorted the
spatial, temporal, and energetic distribution features.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e3831">Magnitudes and MD values calculated for part of the SC catalogue
after <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula> (16 October 1999, sequential number in SC catalogue 21937) from
16 October 1999 (sequential number in SC catalogue 22159) to 21 October 1999
(sequential number in SC catalogue 22697). Average MD values are
calculated for 50-data windows shifted by one data step; 92 % of
earthquakes in this period occurred within a distance of 1.2–60 km from the
epicentre of <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f11.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><label>Figure 12</label><caption><p id="d1e3864">Magnitudes and MD values calculated for part of the SC catalogue
after <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula> (4 April 2010, sequential number in SC catalogue 28129) from
6 April 2010 (sequential number in SC catalogue 28903) to 8 April 2010
(sequential number in SC catalogue 29350). Average MD values were calculated
for 50-data windows shifted by one data step; 99 % of the earthquakes in
this period occurred within a distance of 0.7–60 km from the epicentre of
<inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f12.png"/>

      </fig>

      <?pagebreak page300?><p id="d1e3895">We then carried out a similar analysis for the sequences of relatively small
earthquakes that occurred in periods when no strong earthquakes were
registered. These small earthquakes apparently cannot be regarded as
aftershocks of strong events. In Fig. 13, we present the results of an
analysis of an almost 2-year period of small earthquake activity. This
period began 5 months later, after the <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">5.12</mml:mn></mml:mrow></mml:math></inline-formula> earthquake (1 October 1982,
sequential number in SC catalogue 4591) which was the closest event
exceeding the selected <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula> threshold. According to the proposed view of the
time distribution of aftershocks, it looks very unlikely that the <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">5.12</mml:mn></mml:mrow></mml:math></inline-formula>
earthquake could invoke aftershock activity which lasted 2 years. Thus, in
agreement with our above findings, we can conclude that for the selected
period, the seismic process in the original catalogue is indistinguishable
from the set of catalogues that were randomised using a shuffling procedure
in 60 % of the 50-data windows considered.</p>
      <p id="d1e3931">Figure 14 presents the results for the next part of the catalogue, which
contained relatively small earthquakes in the observation period, which was
far from the occurrence of strong events. A moderately strong earthquake of
<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">5.43</mml:mn></mml:mrow></mml:math></inline-formula> (7 July 2010, sequential number in SC catalogue 31011) occurred
9 months prior to the start of this 10-month long period of small
earthquake activity, which lasted from 7 April 2011 (sequential number in SC
catalogue 31823) to 14 February 2012 (sequential number in SC catalogue 32240). In
this case, we observe that in 75 % of the 50-data windows analysed, the
seismic process in the original catalogue is indistinguishable from the set
of randomised catalogues.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><label>Figure 13</label><caption><p id="d1e3947">Magnitudes and MD values calculated for the non-aftershock part of
the SC catalogue from 7 March 1983 (sequential number in SC catalogue 5000) to
5 February 1985 (sequential number in SC catalogue 6253). Average MD values are
calculated for 50-data windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f13.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14"><?xmltex \currentcnt{14}?><label>Figure 14</label><caption><p id="d1e3959">Magnitudes and MD values calculated for the non-aftershock part of
the SC catalogue from 7 April 2011 (sequential number in SC catalogue 31823)
to 14 February 2012 (sequential number in SC catalogue 32240). Average MD values
are calculated for 50-data windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f14.png"/>

      </fig>

      <p id="d1e3968">In Fig. 15, we present the results for the third part of the catalogue,
which was selected to contain relatively small earthquakes, <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>, in
a period far from strong events (the closest such earthquake of <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula>
occurred more than 5 years earlier, on 16 October 1999, sequential number in
SC catalogue 21937). Two moderately strong <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">5.7</mml:mn></mml:mrow></mml:math></inline-formula> earthquakes (8 December 2001
and 22 February 2002 with sequential numbers in SC catalogue 24491 and 24640)
also occurred a long time before the selected period, which lasted<?pagebreak page301?> from
24 May 2006 to 5 August 2007. Within this period of generation of small
earthquakes, 84 % of the 50-data windows indicated that the seismic
activity in the original catalogue is indistinguishable from the set of
randomised catalogues.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15"><?xmltex \currentcnt{15}?><label>Figure 15</label><caption><p id="d1e4007">Magnitudes and MD values calculated for the non-aftershock part of
the SC catalogue from 24 May 2006 (sequential number in SC catalogue 26259)
to 5 August 2007 (sequential number in SC catalogue 26717). Average MD values
are calculated for 50-data windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f15.png"/>

      </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Testing the stability of the results with respect to the minimum magnitude</title>
      <p id="d1e4026">As can be seen from our results, as assessed based on the ICT(<inline-formula><mml:math id="M212" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M213" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and
ICE(<inline-formula><mml:math id="M214" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) characteristics, the seismic process of generation of relatively small
earthquakes often (although not always) appears random and strongly depends
on the space and time location of these small earthquake sequences. It can
be assumed that if the observed indistinguishability from randomness really
is connected with the features of the seismic process in periods preceding
strong events, then this indistinguishability should also be retained for
higher values of the completeness magnitude threshold. To test this
assumption, we carried out the same analysis for the SC earthquake catalogue
with representative thresholds of <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">3.6</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>. A further increase in the
threshold to <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">5.6</mml:mn></mml:mrow></mml:math></inline-formula> was not feasible, since only 29 earthquakes with
magnitudes larger than <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">5.6</mml:mn></mml:mrow></mml:math></inline-formula> occurred in the SC catalogue during the period
considered in this research.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16" specific-use="star"><?xmltex \currentcnt{16}?><label>Figure 16</label><caption><p id="d1e4097">Average MD values calculated by comparing ICT(<inline-formula><mml:math id="M219" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M220" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M221" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences from the
original SC catalogue and from the set of randomised catalogues
(completeness threshold <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">3.6</mml:mn></mml:mrow></mml:math></inline-formula>). The dotted line corresponds to a significant
difference between windows at <inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. MD values are calculated for 50-data
windows shifted by one data step.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f16.png"/>

      </fig>

      <p id="d1e4150">In Fig. 16, we give results for a completeness magnitude threshold of <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">3.6</mml:mn></mml:mrow></mml:math></inline-formula>.
We can see that the situation for windows in which the seismicity is
indistinguishable from randomness is almost exactly the same as in Fig. 6,
for a completeness magnitude threshold of <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">2.6</mml:mn></mml:mrow></mml:math></inline-formula>. Specifically, in 33 % of
all 50-data windows, the seismic process looks similar to the random process
in catalogues where the dynamical structure of the original seismic process was
intentionally distorted. These random-like windows in the original catalogue
preceded strong events.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><?xmltex \currentcnt{17}?><label>Figure 17</label><caption><p id="d1e4178">Average MD values calculated by comparing ICT(<inline-formula><mml:math id="M226" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M227" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M228" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) sequences from the
original SC catalogue and from the set of randomised catalogues
(completeness threshold <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>). The dotted line corresponds to a significant
difference between windows at <inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>. MD values are calculated for 50-data
windows shifted by one data step. The inset shows results calculated for 30-data windows shifted by one data step.
</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://npg.copernicus.org/articles/26/291/2019/npg-26-291-2019-f17.png"/>

      </fig>

      <p id="d1e4231">As can be seen from Fig. 17, in the case of a higher threshold of <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula> prior to two strong events, <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula>,<?pagebreak page302?> we observe
windows (of 50 data steps) in which the seismic process assessed based on
the  ICT(<inline-formula><mml:math id="M234" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), ICD(<inline-formula><mml:math id="M235" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>), and ICE(<inline-formula><mml:math id="M236" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) characteristics is indistinguishable from the randomised catalogues.
In total, 21 % of the 50-data windows had calculated MDs lower than the
significance threshold value (0.68). Conversely, at a high
representative threshold (<inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>), unlike in the above cases, prior to a
strong <inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula> earthquake, we do not observe 50-data windows in which the
seismic process could be regarded as random.</p>
      <p id="d1e4311">This behaviour is apparently caused by the small number of events above the
<inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula> threshold (below which, as explained above, we regarded earthquakes as
small, Hough and Jones, 1997) in the catalogue, and by the selected length of the
window (50 data steps) for the short data sequence. In the case of 30 data
windows shifted by one data step, we see that prior to the <inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula> earthquake
there are also windows that are indistinguishable from the random catalogues
(see inset in Fig. 17). The proportion of windows showing random behaviour
of the seismic process is 37 %. Summarising the results
in Fig. 17, we can say that shorter windows (apparently in the range 30–50
data steps) seem to be preferable for an analysis such as this. A more
important observation from the results for the high threshold is that the
random-like character of the seismic process observed in windows prior to
strong events apparently is not (or is not always) connected only with small
earthquakes. It seems that long-range correlation features in the seismic
process should not be regarded as being directly related to the sizes of
events.</p>
</sec>
<?pagebreak page303?><sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Conclusions</title>
      <p id="d1e4344">We have investigated the variability in the regularity of the seismic
process, based on its spatial, temporal, and energetic characteristics. For
this purpose, we used an SC earthquake catalogue over the period 1975 to
2017. Our method of analysis was a combination of multivariate Mahalanobis
distance calculation and surrogate data testing. We carried out a
multivariate assessment of changes in the regularity of the seismic process,
based on increments of cumulative times, increments of cumulative distances,
and increments of cumulative seismic energies calculated from the SC
earthquake catalogue.</p>
      <p id="d1e4347">In order to assess the ability of the multivariate approach used here to
discriminate between different conditions of dynamical systems, we used two
3-D models in which the dynamical features were changed from a more regular
form to more randomised conditions by adding a certain degree of noise.</p>
      <p id="d1e4350">It was shown that in about a third of the analysed 50-data windows, the
original seismic process is indistinguishable from a random process by the
features of its temporal, spatial, and energetic variability. Prior to the
occurrence of strong earthquakes, in periods in which there are events with
relatively small magnitudes (<inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">4.6</mml:mn></mml:mrow></mml:math></inline-formula>), the percentage of windows in
which the seismic process is indistinguishable from a random process increases
to 60 %–80 %. At the same time, during periods of aftershock activity,
the process of small earthquake generation becomes more regular in all of
the windows considered and thus is strongly differentiated from the
randomised catalogues.</p>
      <p id="d1e4366">Based on the results of our analysis, we conclude that the seismic process
cannot in general be regarded either as completely random or as completely
regular (deterministic). Instead, we can say that the dynamics of the
seismic process undergoes strong time-dependent changes. In other words, the
regularity of the seismic process, as assessed based on the temporal,
spatial, and energetic distributions, changes over time.</p>
      <p id="d1e4370">It was also shown that in some periods, the seismic process appears to be
closer to randomness, while in other cases it becomes closer to regular
behaviour. More specifically, in periods of relatively low earthquake
generation activity (i.e. with smaller energy release), the seismic process
looks more random, while in periods of occurrence of strong events, followed
by a series of aftershocks, it shows significant deviation from randomness
(i.e. the extent of regularity essentially increases). The period for which
this deviation from random behaviour lasts depends on the amount of seismic
energy released by the strong earthquake. The results obtained here
from a multivariable assessment of the dynamical features of the seismic
process are in accordance with our previous findings on the dynamical
changes in the temporal distribution of earthquakes (Matcharashvili et al.,
2018).</p>
      <p id="d1e4373">It should be underlined that the occurrence in July 2019 (during the
editorial process of our manuscript in NPG) of two strong earthquakes, <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">6.4</mml:mn></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">7.1</mml:mn></mml:mrow></mml:math></inline-formula>, in the considered catalogue area additionally convinced us that
random-like behaviour of seismic processes may indeed be regarded as one of the
possible precursory markers of strong earthquakes.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e4402">Used in this research, seismic data are available from the catalogue which is accessible from the official site (<uri>http://www.isc.ac.uk/iscbulletin/search/catalogue/</uri>) as is mentioned in the data section. Used model data sets in case of interest can be easily modelled as they are described in Sect. 4.1 and 4.2.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e4411">The authors contributed in accordance with their competence in the research subject. The first author TM was responsible for all aspects of research and manuscript preparation. An immense contribution by ZC helped to ensure a high mathematical and modelling level of research, and NZ contributed through programming, data analysis, and active participation in the manuscript preparation.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e4417">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4423">The authors acknowledge the useful comments of the reviewers, Eleftheria Papadimitriou and Antonella Peresan.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e4428">This research was supported by the Shota Rustaveli National Science Foundation (SRNSF) (“Investigation of the dynamics of the
temporal distribution of earthquakes” (grant no.   217838)).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e4435">This paper was edited by Ilya Zaliapin and reviewed by Eleftheria Papadimitriou and Antonella Peresan.</p>
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    <!--<article-title-html>Mahalanobis distance-based recognition of changes in the dynamics of a seismic process</article-title-html>
<abstract-html><p>In the present work, we aim to analyse the regularity of
a seismic process based on its spatial, temporal, and energetic
characteristics. Increments of cumulative times, increments of cumulative
distances, and increments of cumulative seismic energies are calculated from
an earthquake catalogue for southern California from 1975 to 2017.</p><p>As the method of analysis, we use the multivariate Mahalanobis distance
calculation, combined with a surrogate data testing procedure that is often
used for the testing of non-linear structures in complex data sets. Before
analysing the dynamical features of the seismic process, we tested the used
approach for two different 3-D models in which the dynamical features were
changed from more regular to more randomised conditions by adding a certain
degree of noise.</p><p>An analysis of the variability in the extent of regularity of the seismic
process was carried out for different completeness magnitude thresholds.</p><p>The results of our analysis show that in about a third of all the 50-data
windows the original seismic process was indistinguishable from a random
process based on its features of temporal, spatial, and energetic
variability. It was shown that prior to the occurrence of strong earthquakes,
mostly in periods of generation of relatively small earthquakes, the
percentage of windows in which the seismic process is indistinguishable from
a random process increases (to 60&thinsp;%–80&thinsp;%). During periods of aftershock
activity, the process of small earthquake generation became regular in all
of the windows considered, and thus was markedly different from the
randomised catalogues.</p><p>In some periods within the catalogue, the seismic process appeared to be
closer to randomness, while in other cases it became closer to a regular behaviour. More specifically, in periods of relatively
decreased earthquake generation activity (with low energy release), the
seismic process appears to be random, while during periods of occurrence of
strong events, followed by series of aftershocks, significant deviation from
randomness is shown, i.e. the extent of regularity markedly increases. The
period for which such deviation from random behaviour lasts depends on the
amount of seismic energy released by the strong earthquake.</p></abstract-html>
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Matcharashvili, T., Chelidze, T., and Javakhishvili, Z.: Nonlinear analysis of magnitude and interevent time interval sequences for earthquakes of the Caucasian region, Nonlin. Processes Geophys., 7, 9–20, <a href="https://doi.org/10.5194/npg-7-9-2000" target="_blank">https://doi.org/10.5194/npg-7-9-2000</a>, 2000.
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Detecting differences in dynamics of small earthquakes temporal distribution
before and after large events, Comput. Geosci., 28, 693–700, 2002.
</mixed-citation></ref-html>
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E.: Analysis of long-term variation of the annual number of warmer and
colder days using Mahalanobis distance metrics – A case study for Athens,
Physica A, 487, 22–31, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib36"><label>36</label><mixed-citation>
Matcharashvili, T., Hatano, T., Chelidze, T., and Zhukova, N.: Simple statistics for complex Earthquake time distributions, Nonlin. Processes Geophys., 25, 497–510, <a href="https://doi.org/10.5194/npg-25-497-2018" target="_blank">https://doi.org/10.5194/npg-25-497-2018</a>, 2018.
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Differences of precursory seismic energy release for the 2007 effusive
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renormalization group theory of earthquakes: Implications for earthquake
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technology system, John Wiley and Sons, Inc., 2002.

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earthquake interevent time distribution, Phys. Rev. Lett., 102, 168501,
<a href="https://doi.org/10.1103/PhysRevLett.102.168501" target="_blank">https://doi.org/10.1103/PhysRevLett.102.168501</a>, 2009.
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inter-occurrence times of earthquakes, J. Seismol., 2,    351, <a href="https://doi.org/10.1023/A:1009774819512" target="_blank">https://doi.org/10.1023/A:1009774819512</a>,  1998.
</mixed-citation></ref-html>--></article>
