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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-21-1113-2014</article-id>
<title-group>
<article-title>Long-term changes in the north–south asymmetry of solar activity: a nonlinear dynamics characterization using visibility graphs</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zou</surname>
<given-names>Y.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Donner</surname>
<given-names>R. V.</given-names>
<ext-link>https://orcid.org/0000-0001-7023-6375</ext-link>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Marwan</surname>
<given-names>N.</given-names>
<ext-link>https://orcid.org/0000-0003-1437-7039</ext-link>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Small</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kurths</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Physics, East China Normal University, 200062 Shanghai, China</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Potsdam Institute for Climate Impact Research, P.O. Box 60 12 03, 14412 Potsdam, Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Max Planck Institute for Biogeochemistry, Hans-Knöll-Str. 10, 07745 Jena, Germany</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>School of Mathematics and Statistics, University of Western Australia, Crawley, WA 6009, Australia</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Department of Physics, Humboldt University Berlin, Newtonstr. 15, 12489 Berlin, Germany</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>Institute for Complex Systems and Mathematical Biology, University of Aberdeen, Aberdeen, AB243UE, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>24</day>
<month>11</month>
<year>2014</year>
</pub-date>
<volume>21</volume>
<issue>6</issue>
<fpage>1113</fpage>
<lpage>1126</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2014 Y. Zou et al.</copyright-statement>
<copyright-year>2014</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://npg.copernicus.org/articles/21/1113/2014/npg-21-1113-2014.html">This article is available from https://npg.copernicus.org/articles/21/1113/2014/npg-21-1113-2014.html</self-uri>
<self-uri xlink:href="https://npg.copernicus.org/articles/21/1113/2014/npg-21-1113-2014.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/21/1113/2014/npg-21-1113-2014.pdf</self-uri>
<abstract>
<p>Solar activity is characterized by complex dynamics superimposed onto an almost
periodic, approximately 11-year cycle. One of its main features is the presence of a
marked, time-varying hemispheric asymmetry, the deeper reasons for which have
not yet been completely uncovered. Traditionally, this asymmetry has been
studied by considering amplitude and phase differences. Here, we use
visibility graphs, a novel tool of nonlinear time series analysis, to obtain
complementary information on hemispheric asymmetries in dynamical properties.
Our analysis provides deep insights into the potential and limitations of
this method, revealing a complex interplay between factors relating to
statistical and dynamical properties, i.e., effects due to the probability
distribution and the regularity of observed fluctuations. We demonstrate that
temporal changes in the hemispheric predominance of the graph properties lag
those directly associated with the total hemispheric sunspot areas. Our
findings open a new dynamical perspective on studying the north–south
sunspot asymmetry, which is to be further explored in future work.</p>
</abstract>
<counts><page-count count="14"/></counts>
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>11305062, 11135001, 11075056</award-id>
</award-group>
<award-group id="gs2">
<funding-source></funding-source>
<award-id>20130076120003</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
<body/>
<back>
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