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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-24-2735-2006</article-id>
<title-group>
<article-title>On the scaling of waiting-time distributions of the negative IMF &lt;i&gt;B&lt;sub&gt;z&lt;/sub&gt;&lt;/i&gt; component</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>D&apos;Amicis</surname>
<given-names>R.</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>Bruno</surname>
<given-names>R.</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>Bavassano</surname>
<given-names>B.</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>Carbone</surname>
<given-names>V.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sorriso-Valvo</surname>
<given-names>L.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Istituto di Fisica dello Spazio Interplanetario (INAF), 00133 Roma, Italy</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Dipartimento di Fisica Università della Calabria, 87036 Rende (Cs), Italy</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Liquid Crystal Laboratory, INFM/CNR, 87030 Rende (Cs), Italy</addr-line>
</aff>
<pub-date pub-type="epub">
<day>20</day>
<month>10</month>
<year>2006</year>
</pub-date>
<volume>24</volume>
<issue>10</issue>
<fpage>2735</fpage>
<lpage>2741</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/24/2735/2006/angeo-24-2735-2006.pdf">The full text article is available as a PDF file from http://www.ann-geophys.net/24/2735/2006/angeo-24-2735-2006.pdf</self-uri>
<abstract>
<p>Statistics associated with the fluctuations in solar wind parameters show a
remarkable dependence on the solar activity phase.
In particular, we focus our attention on the waiting-time statistics
governing the MHD fluctuations of the z-component of the interplanetary
magnetic field, which are important within the framework of the Sun-Earth connections, and
briefly discuss the preliminary results.
Data from several spacecrafts, covering different phases of the solar cycle and
different radial distances, are used. We found that propagating Alfvénic
fluctuations and convected structures strongly influence the
statistics which vary from quasi-Poissonian to power law.</p>
</abstract>
<counts><page-count count="7"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
<title>References</title>
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</article>