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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-11-303-2004</article-id>
<title-group>
<article-title>Analysis of the geomagnetic activity of the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index and self-affine fractals using wavelet transforms</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wei</surname>
<given-names>H. L.</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>Billings</surname>
<given-names>S. 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>Balikhin</surname>
<given-names>M.</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 Automatic Control and Systems Engineering, University of Sheffield, Mappin Street, Sheffield, S1 3JD, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>18</day>
<month>06</month>
<year>2004</year>
</pub-date>
<volume>11</volume>
<issue>3</issue>
<fpage>303</fpage>
<lpage>312</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 H. L. Wei et al.</copyright-statement>
<copyright-year>2004</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
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<self-uri xlink:href="https://npg.copernicus.org/articles/11/303/2004/npg-11-303-2004.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/11/303/2004/npg-11-303-2004.pdf</self-uri>
<abstract>
<p>The geomagnetic activity of the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index is analyzed using wavelet transforms
and it is shown that the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index possesses properties associated with
self-affine fractals. For example, the power spectral density obeys a
power-law dependence on frequency, and therefore the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index can be viewed as
a self-affine fractal dynamic process. In fact, the behaviour of the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index,
with a Hurst exponent &lt;i&gt;H&lt;/i&gt;&amp;asymp;0.5 (power-law exponent &amp;beta;&amp;asymp;2) at
high frequency, is similar to that of Brownian motion. Therefore, the
dynamical invariants of the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index may be described by a potential Brownian
motion model. Characterization of the geomagnetic activity has been studied
by analysing the geomagnetic field using a wavelet covariance technique. The
wavelet covariance exponent provides a direct effective measure of the
strength of persistence of the &lt;i&gt;D&lt;sub&gt;st&lt;/sub&gt;&lt;/i&gt; index. One of the advantages of wavelet
analysis is that many inherent problems encountered in Fourier transform
methods, such as windowing and detrending, are not necessary.</p>
</abstract>
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