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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-23-3685-2005</article-id>
<title-group>
<article-title>Under and over-adiabatic electrons through a perpendicular collisionless shock: theory versus simulations</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Savoini</surname>
<given-names>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>Lembège</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>Krasnosselskhik</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>Kuramitsu</surname>
<given-names>Y.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>CETP/UVSQ, 32–40, Avenue de l’Europe, 78140 Vélizy, France</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>LPCE/CNRS, 3a, Avenue de la recherche scientifique, 45071 Orléans la Source, France</addr-line>
</aff>
<pub-date pub-type="epub">
<day>23</day>
<month>12</month>
<year>2005</year>
</pub-date>
<volume>23</volume>
<issue>12</issue>
<fpage>3685</fpage>
<lpage>3698</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2005 P. Savoini et al.</copyright-statement>
<copyright-year>2005</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/23/3685/2005/angeo-23-3685-2005.html">This article is available from https://angeo.copernicus.org/articles/23/3685/2005/angeo-23-3685-2005.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/23/3685/2005/angeo-23-3685-2005.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/23/3685/2005/angeo-23-3685-2005.pdf</self-uri>
<abstract>
<p>Test particle simulations are performed in order to analyze in detail the
dynamics of transmitted electrons through a supercritical, strictly
perpendicular, collisionless shock. In addition to adiabatic particles, two
distinct nonadiabatic populations are observed surprisingly: (i) first, an
&lt;I&gt;over-adiabatic&lt;/I&gt; population characterized by an increase in the gyrating
velocity higher than that expected from the conservation of the magnetic
moment &amp;micro;, and &lt;I&gt;(ii)&lt;/I&gt; second, an &lt;I&gt;under-adiabatic&lt;/I&gt; population
characterized by a decrease in this velocity. Results show that both
nonadiabatic populations have their pitch angle more aligned along the magnetic
field
 than the adiabatic one at the time these hit the shock front. The formation of
 &quot;&lt;I&gt;under&lt;/I&gt;&quot; and &quot;&lt;I&gt;over-adiabatic&lt;/I&gt;&quot; particles strongly depends on
their local injection conditions through the large amplitude cross-shock
potential present
 within the shock front.
A simplified theoretical model validates these results and points out the
important role of the electric field as seen by the electrons. A classification
shows that both nonadiabatic electrons are issued from the core part of the
upstream distributionÊ function. In contrast, suprathermal and tail electrons
only contribute to the adiabatic population; nevertheless, the core part of the
upstream distribution contributes at a lower percentage to the adiabatic
electrons. &lt;I&gt;Under-adiabatic&lt;/I&gt; electrons are characterized by small
injection angles &amp;theta;&lt;sub&gt;&lt;i&gt;inj&lt;/i&gt;&lt;/sub&gt;&amp;le;90&amp;deg;, whereas
&quot;&lt;I&gt;over-adiabatic&lt;/I&gt;&quot; particles have high injection angles
&amp;theta;&lt;sub&gt;&lt;i&gt;inj&lt;/i&gt;&lt;/sub&gt;&amp;gt;90&amp;deg; (where &amp;theta;&lt;sub&gt;&lt;i&gt;inj&lt;/i&gt;&lt;/sub&gt; is the angle between the local gyrating
velocity vector and the shock normal).</p>
</abstract>
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