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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-23-867-2005</article-id>
<title-group>
<article-title>Latitude-energy structure of multiple ion beamlets in Polar/TIMAS data in plasma sheet boundary layer and boundary plasma sheet below 6 &lt;i&gt;R&lt;sub&gt;E&lt;/sub&gt;&lt;/i&gt; radial distance: basic properties and statistical analysis</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Janhunen</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>Olsson</surname>
<given-names>A.</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>Peterson</surname>
<given-names>W. K.</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>Menietti</surname>
<given-names>J. D.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Finnish Meteorological Institute, Space Research, Helsinki, Finland</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Swedish Institute of Space Physics, Uppsala, Sweden</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>LASP, University of Colorado, Boulder, Colorado, USA</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>University of Iowa, Iowa, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>03</month>
<year>2005</year>
</pub-date>
<volume>23</volume>
<issue>3</issue>
<fpage>867</fpage>
<lpage>876</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>
<self-uri xlink:href="http://www.ann-geophys.net/23/867/2005/angeo-23-867-2005.html">This article is available from http://www.ann-geophys.net/23/867/2005/angeo-23-867-2005.html</self-uri>
<self-uri xlink:href="http://www.ann-geophys.net/23/867/2005/angeo-23-867-2005.pdf">The full text article is available as a PDF file from http://www.ann-geophys.net/23/867/2005/angeo-23-867-2005.pdf</self-uri>
<abstract>
<p>Velocity dispersed ion signatures (VDIS) occurring at the plasma
sheet boundary layer (PSBL) are a well reported feature. Theory has, however,
predicted the existence of multiple ion beamlets, similar to VDIS,
in the boundary plasma sheet (BPS), i.e. at latitudes below the
PSBL. In this study we show evidence for
the multiple ion beamlets in Polar/TIMAS ion data and basic
properties of the ion beamlets will be presented. Statistics of the
occurrence frequency of ion multiple beamlets show that they are most
common in the midnight MLT sector and for altitudes above 4 &lt;i&gt;R&lt;sub&gt;E&lt;/sub&gt;&lt;/i&gt;,
while at low altitude (&amp;le;3 &lt;i&gt;R&lt;sub&gt;E&lt;/sub&gt;&lt;/i&gt;), single beamlets at PSBL (VDIS) are more
common. Distribution functions of ion beamlets in velocity space
have recently been shown to correspond to 3-dimensional hollow spheres,
containing a large amount of free energy.  We also study correlation with ~100
Hz waves and electron anisotropies and consider the
possibility that ion beamlets correspond to stable auroral arcs.</p>
</abstract>
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</article-meta>
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