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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-27-1027-2009</article-id>
<title-group>
<article-title>Formation of lower-hybrid solitary structures by modulational interaction between lower-hybrid and dispersive Alfvén waves</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Hall</surname>
<given-names>J. O.</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>Stenberg</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>Eriksson</surname>
<given-names>A. I.</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>André</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Swedish Institute of Space Physics, Uppsala, Sweden</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>present address: Swedish Defence Research Agency, Stockholm, Sweden</addr-line>
</aff>
<pub-date pub-type="epub">
<day>02</day>
<month>03</month>
<year>2009</year>
</pub-date>
<volume>27</volume>
<issue>3</issue>
<fpage>1027</fpage>
<lpage>1033</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2009 J. O. Hall et al.</copyright-statement>
<copyright-year>2009</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/27/1027/2009/angeo-27-1027-2009.html">This article is available from https://angeo.copernicus.org/articles/27/1027/2009/angeo-27-1027-2009.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/27/1027/2009/angeo-27-1027-2009.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/27/1027/2009/angeo-27-1027-2009.pdf</self-uri>
<abstract>
<p>We investigate the possibility that lower-hybrid solitary structures
  (LHSS), which are frequently observed in the Earth&apos;s ionosphere and
  magnetosphere, are formed as a result of a modulational interaction
  between lower-hybrid and dispersive Alfvén waves of initially
  small amplitude. A large amplitude lower-hybrid pump wave can
  excite density structures with length scales transverse to the
  geomagnetic field of the order of the ion gyroradius via a
  modulational instability. The structure formation in the nonlinear
  stage of the instability is investigated by numerical solutions of
  the governing equations, using plasma parameters relevant for
  LHSS observations in the upper ionosphere and in the magnetosphere.
  The numerical solutions reveal that the
  lower-hybrid waves become self-localized inside cylindrically
  symmetric (with respect to the ambient magnetic field) density
  cavities, in qualitative agreement with observations. Our model
  includes thermal electron effects but shows no stabilization at the
  ion sound gyroradius, suggesting that any preference of observed
  LHSS for that perpendicular scale likely is due to processes
  arresting the cavity collapse.</p>
</abstract>
<counts><page-count count="7"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
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</back>
</article>