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<front>
<journal-meta>
<journal-id journal-id-type="publisher">NPG</journal-id>
<journal-title-group>
<journal-title>Nonlinear Processes in Geophysics</journal-title>
<abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1607-7946</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/npg-10-65-2003</article-id>
<title-group>
<article-title>Some theoretical models for solitary structures of boundary layer waves</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lakhina</surname>
<given-names>G. 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>Tsurutani</surname>
<given-names>B. T.</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>Singh</surname>
<given-names>S. V.</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>Reddy</surname>
<given-names>R. V.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Indian Institute of Geomagnetism, Colaba, Mumbai, India</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Indian Institute of Geomagnetism, Colaba, Mumbai, India</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>04</month>
<year>2003</year>
</pub-date>
<volume>10</volume>
<issue>1/2</issue>
<fpage>65</fpage>
<lpage>73</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2003 G. S. Lakhina et al.</copyright-statement>
<copyright-year>2003</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
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<self-uri xlink:href="https://npg.copernicus.org/articles/10/65/2003/npg-10-65-2003.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/10/65/2003/npg-10-65-2003.pdf</self-uri>
<abstract>
<p>Solitary
      electrostatic structures have been observed in and around auroral zone
      field lines at various altitudes ranging from close to the ionosphere, to
      the magnetopause low-latitude boundary layer (LLBL) and cusp on the
      dayside, and to the plasma sheet boundary layer on the night-side. In this
      review, various models based on solitons/double layers and BGK modes or
      phase space holes are discussed in order to explain the characteristics of
      these solitary structures.</p>
</abstract>
<counts><page-count count="9"/></counts>
</article-meta>
</front>
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