<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="3.0" xml:lang="en">
<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-19-1567-2001</article-id>
<title-group>
<article-title>Four point measurements of electrons using PEACE in the high-altitude cusp</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Taylor</surname>
<given-names>M. G. G. T.</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>Fazakerley</surname>
<given-names>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>Krauklis</surname>
<given-names>I. C.</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>Owen</surname>
<given-names>C. J.</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>Travnicek</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dunlop</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Carter</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>Coates</surname>
<given-names>A. J.</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>Szita</surname>
<given-names>S.</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>Watson</surname>
<given-names>G.</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>Wilson</surname>
<given-names>R. J.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Mullard Space Science Laboratory, University College London, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institute of Atmospheric Physics, The Academy of Sciences of the Czech Republic</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Imperial College of Science Technology and Medicine, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>09</month>
<year>2001</year>
</pub-date>
<volume>19</volume>
<issue>10/12</issue>
<fpage>1567</fpage>
<lpage>1578</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2001 M. G. G. T. Taylor et al.</copyright-statement>
<copyright-year>2001</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/19/1567/2001/angeo-19-1567-2001.html">This article is available from https://angeo.copernicus.org/articles/19/1567/2001/angeo-19-1567-2001.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/19/1567/2001/angeo-19-1567-2001.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/19/1567/2001/angeo-19-1567-2001.pdf</self-uri>
<abstract>
<p>We present examples of
 electron measurements from the PEACE instruments on the Cluster spacecraft in
 the high-latitude, high-altitude region of the Earth’s magnetosphere. Using
 electron density and energy spectra measurements, we examine two cases where
 the orbit of the Cluster tetrahedron is outbound over the northern hemisphere,
 in the afternoon sector approaching the magnetopause. Data from the
 magnetometer is also used to pinpoint the position of the spacecraft with
 respect to magnetospheric boundaries. This preliminary work specifically
 highlights the benefit of the multipoint measurement capability of the Cluster
 mission. In the first case, we observe a small-scale spatial structure within
 the magnetopause boundary layer. The Cluster spacecraft initially straddle a
 boundary, characterised by a discontinuous change in the plasma population,
 with a pair of spacecraft on either side. This is followed by a complete
 crossing of the boundary by all four spacecraft. In the second case, Cluster
 encounters an isolated region of higher energy electrons within the cusp. The
 characteristics of this region are consistent with a trapped boundary layer
 plasma sheet population on closed magnetospheric field lines. However, a
 boundary motion study indicates that this region convects past Cluster, a
 characteristic more consistent with open field lines. An interpretation of this
 event in terms of the motion of the cusp boundary region is presented.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words. &lt;/b&gt;Magnetospheric physics
 (magnetopause, cusp and boundary layers; solar wind-magnetosphere interactions)</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
</front>
<body/>
<back>
</back>
</article>