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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ANGEO</journal-id>
<journal-title-group>
<journal-title>Annales Geophysicae</journal-title>
<abbrev-journal-title abbrev-type="publisher">ANGEO</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Ann. Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1432-0576</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/angeo-21-1975-2003</article-id>
<title-group>
<article-title>Geometrical characteristics of magnetospheric energetic ion time series: evidence for low dimensional chaos</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pavlos</surname>
<given-names>G. P.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Athanasiu</surname>
<given-names>M. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Rigas</surname>
<given-names>A. G.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sarafopoulos</surname>
<given-names>D. V.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sarris</surname>
<given-names>E. T.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Electrical and Computer Engineering, Demokritos Univercity of Thrace, 67100 Xanthi, Greece</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>09</month>
<year>2003</year>
</pub-date>
<volume>21</volume>
<issue>9</issue>
<fpage>1975</fpage>
<lpage>1993</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2003 G. P. Pavlos et al.</copyright-statement>
<copyright-year>2003</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>
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<self-uri xlink:href="https://angeo.copernicus.org/articles/21/1975/2003/angeo-21-1975-2003.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/21/1975/2003/angeo-21-1975-2003.pdf</self-uri>
<abstract>
<p>In the first part of the
 paper we study the geometrical characteristics of the magnetospheric ions’
 time series in the reconstructed phase space by using the SVD extended chaotic
 analysis, and we test the strong null hypothesis supposing that the ions’
 time series is caused by a linear stochastic process perturbed by a static
 nonlinear distortion. The SVD reconstructed spectrum of the ions’ signal
 reveals a strong component of high dimensional, external coloured noise, as
 well as an internal low dimensional nonlinear deterministic component. Also,
 the stochastic Lorenz system produced by coloured noise perturbation of the
 deterministic Lorenz system was used as an archetype model in comparison with
 the dynamics of the magnetrospheric ions.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words. &lt;/b&gt;Magnetospheric physics
 (energetic particles) – Radio science (nonlinear phenomena)</p>
</abstract>
<counts><page-count count="19"/></counts>
</article-meta>
</front>
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