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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-20-445-2002</article-id>
<title-group>
<article-title>Energetic particle observations at the subsolar magnetopause</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Eccles</surname>
<given-names>A. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fritz</surname>
<given-names>T. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Boston University Center for Space Physics, Boston MA, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Correspondence to: T. A. Fritz (fritz@bu.edu)</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>04</month>
<year>2002</year>
</pub-date>
<volume>20</volume>
<issue>4</issue>
<fpage>445</fpage>
<lpage>460</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2002 A. A. Eccles</copyright-statement>
<copyright-year>2002</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/20/445/2002/angeo-20-445-2002.html">This article is available from https://angeo.copernicus.org/articles/20/445/2002/angeo-20-445-2002.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/20/445/2002/angeo-20-445-2002.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/20/445/2002/angeo-20-445-2002.pdf</self-uri>
<abstract>
<p>The pitch-angle distributions (PAD) of
 energetic particles are examined as the ISEE-1 satellite crosses the Earth’s
 magnetopause near the subsolar point. The investigation focuses on the possible
 existence of a particular type of distribution that would be associated with a
 source of energetic particles in the high-latitude magnetosphere. PADs,
 demonstrating broad, persistent field-aligned fluxes filling a single
 hemisphere (upper/northern or lower/southern), were observed just sunward of
 the magnetopause current layer for an extended period of many minutes. These
 distributions are a direct prediction of a possible source of energetic
 particles located in the high altitude dayside cusp and we present five
 examples in detail of the three-dimensional particle distributions to
 demonstrate their existence. From these results, other possible causes of such
 PADs are examined.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words.&lt;/b&gt; Magnetospheric physics (energetic
 particles, precipitating; magnetopause, cusp and boundary layers;
 magnetospheric configuration and dynamics)</p>
</abstract>
<counts><page-count count="16"/></counts>
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