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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-29-2253-2011</article-id>
<title-group>
<article-title>Proton/electron temperature ratio in the magnetotail</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Artemyev</surname>
<given-names>A. 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>Baumjohann</surname>
<given-names>W.</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>Petrukovich</surname>
<given-names>A. 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>Nakamura</surname>
<given-names>R.</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>Dandouras</surname>
<given-names>I.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</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>Fazakerley</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Space Research Institute, Russian Academy of Sciences, Moscow, Russia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Space Research Institute, Austrian Academy of Sciences, Graz, Austria</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>IRAP, University of Toulouse, UPS-OMP, Toulouse, France</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>CNRS, IRAP, 9 Ave. Colonel Roche, BP 44346, 31028 Toulouse cedex 4, France</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Mullard Space Science Laboratory, London, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>15</day>
<month>12</month>
<year>2011</year>
</pub-date>
<volume>29</volume>
<issue>12</issue>
<fpage>2253</fpage>
<lpage>2257</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2011 A. V. Artemyev et al.</copyright-statement>
<copyright-year>2011</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://angeo.copernicus.org/articles/29/2253/2011/angeo-29-2253-2011.html">This article is available from https://angeo.copernicus.org/articles/29/2253/2011/angeo-29-2253-2011.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/29/2253/2011/angeo-29-2253-2011.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/29/2253/2011/angeo-29-2253-2011.pdf</self-uri>
<abstract>
<p>We study the temperature ratio of protons and electrons based on statistics
of Cluster observations in the Earth&apos;s magnetotail from 2001 to 2004. During
these years, from June to November, the Cluster spacecraft visited the plasma
sheet at the distance &lt;I&gt;r&lt;/I&gt;~&amp;minus;19 &lt;I&gt;R&lt;/I&gt;&lt;sub&gt;E&lt;/sub&gt;. We use proton and electron moments
collected in the central region of the plasma sheet (|&lt;I&gt;Z&lt;/I&gt;|&amp;lt;5 &lt;I&gt;R&lt;/I&gt;&lt;sub&gt;E&lt;/sub&gt;). We find an
average ratio of proton and electron temperatures ⟨&lt;I&gt;T&lt;/I&gt;&lt;sub&gt;p&lt;/sub&gt;/&lt;I&gt;T&lt;/I&gt;&lt;sub&gt;e&lt;/sub&gt; ⟩
&amp;approx; 3.5. The dependence of &lt;I&gt;T&lt;/I&gt;&lt;sub&gt;p&lt;/sub&gt; on &lt;I&gt;T&lt;/I&gt;&lt;sub&gt;e&lt;/sub&gt; can be approximated by the
power-law function: &lt;I&gt;T&lt;/I&gt;&lt;sub&gt;p&lt;/sub&gt; &amp;approx; 11&lt;I&gt;T&lt;/I&gt;&lt;sub&gt;e&lt;/sub&gt;&lt;sup&gt;0.62&lt;/sup&gt;, where &lt;I&gt;T&lt;/I&gt;&lt;sub&gt;p&lt;/sub&gt; and &lt;I&gt;T&lt;/I&gt;&lt;sub&gt;e&lt;/sub&gt; are
measured in MK. A previous reported ratio ⟨&lt;I&gt;T&lt;/I&gt;&lt;sub&gt;p&lt;/sub&gt;/&lt;I&gt;T&lt;/I&gt;&lt;sub&gt;e&lt;/sub&gt; ⟩ ~ 7 is
limited to small electron temperatures &amp;lt;20 MK. The observations with the
high electron temperature correspond to smaller values of the electron
density and larger values of the proton and electron bulk velocities. A
correlation between &lt;I&gt;T&lt;/I&gt;&lt;sub&gt;e&lt;/sub&gt; and curlometer current density is not found.</p>
</abstract>
<counts><page-count count="5"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>