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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>
</journal-title-group>
<issn pub-type="epub">1432-0576</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/angeo-29-1331-2011</article-id>
<title-group>
<article-title>The correlation between solar and geomagnetic activity – Part 1: Two-term decomposition of geomagnetic activity</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Du</surname>
<given-names>Z. L.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China</addr-line>
</aff>
<pub-date pub-type="epub">
<day>05</day>
<month>08</month>
<year>2011</year>
</pub-date>
<volume>29</volume>
<issue>8</issue>
<fpage>1331</fpage>
<lpage>1340</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
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<self-uri xlink:href="http://www.ann-geophys.net/29/1331/2011/angeo-29-1331-2011.pdf">The full text article is available as a PDF file from http://www.ann-geophys.net/29/1331/2011/angeo-29-1331-2011.pdf</self-uri>
<abstract>
<p>By analyzing the logarithmic relationship between geomagnetic
activity as represented by the annual &lt;I&gt;aa&lt;/I&gt; index and solar
magnetic field activity as represented by the annual sunspot
number (&lt;I&gt;R&lt;/I&gt;&lt;sub&gt;z&lt;/sub&gt;) during the period 1844–2010, &lt;I&gt;aa&lt;/I&gt; is
shown to lie in between two lines defined solely by
&lt;I&gt;R&lt;/I&gt;&lt;sub&gt;z&lt;/sub&gt;. Two ways can be used to decompose the &lt;I&gt;aa&lt;/I&gt; index
into two components. One is decomposing &lt;I&gt;aa&lt;/I&gt; into the sum of the
baseline (&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;b&lt;/sub&gt;) and the remainder (&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;u&lt;/sub&gt;)
with a null correlation. Another is dividing the top-line
(&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;t&lt;/sub&gt;) into the sum of &lt;I&gt;aa&lt;/I&gt; and the remainder
(&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;d&lt;/sub&gt;) with a null correlation. The first decomposition
is similar to the traditional one. The second decomposition
implies a nonlinear relationship of &lt;I&gt;aa&lt;/I&gt; with &lt;I&gt;R&lt;/I&gt;&lt;sub&gt;z&lt;/sub&gt;
(&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;t&lt;/sub&gt;) and a decay process (&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;d&lt;/sub&gt;).
Therefore,
&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;t&lt;/sub&gt;=&lt;I&gt;aa&lt;/I&gt;+&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;d&lt;/sub&gt;=&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;b&lt;/sub&gt;+&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;u&lt;/sub&gt;+&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;d&lt;/sub&gt;:
(i) &lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;t&lt;/sub&gt; is related to the solar energy potential of
generating geomagnetic activity (associated with &lt;I&gt;R&lt;/I&gt;&lt;sub&gt;z&lt;/sub&gt;);
(ii) &lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;b&lt;/sub&gt; is related to transient phenomena; (iii)
&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;u&lt;/sub&gt; is related to recurrent phenomena; and (iv)
&lt;I&gt;aa&lt;/I&gt;&lt;sub&gt;d&lt;/sub&gt; is related to the energy loss in the transmission
from solar surface to the magnetosphere and ionosphere that failed
to generate geomagnetic activity.</p>
</abstract>
<counts><page-count count="10"/></counts>
</article-meta>
</front>
<body/>
<back>
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