<?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">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-11-421-2004</article-id>
<title-group>
<article-title>Trans-sonic cusped shaped, periodic waves and solitary waves of the electrostatic ion-cyclotron type</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>McKenzie</surname>
<given-names>J. F.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Doyle</surname>
<given-names>T. B.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Max-Planck-Institute for Solarsystems Research, Katlenburg-Lindau, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>School of Physics &amp; School of Mathematical and Statistical Sciences, Univ. of KwaZulu-Natal, Durban, 4041, South Africa</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Physics, University of Alabama at Huntsville, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>24</day>
<month>09</month>
<year>2004</year>
</pub-date>
<volume>11</volume>
<issue>4</issue>
<fpage>421</fpage>
<lpage>425</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 J. F. McKenzie</copyright-statement>
<copyright-year>2004</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>
<self-uri xlink:href="https://npg.copernicus.org/articles/11/421/2004/npg-11-421-2004.html">This article is available from https://npg.copernicus.org/articles/11/421/2004/npg-11-421-2004.html</self-uri>
<self-uri xlink:href="https://npg.copernicus.org/articles/11/421/2004/npg-11-421-2004.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/11/421/2004/npg-11-421-2004.pdf</self-uri>
<abstract>
<p>By adopting an essentially fluid dynamic viewpoint we derive the
wave structure equation for stationary, fully nonlinear,
electrostatic, ion-cyclotron waves.  The existence of two
fundamental constants of the motion, namely, conservation of
momentum flux parallel to the ambient magnetic field, and energy
flux parallel to the direction of wave propagation, enables the wave
structure equation to be reduced to a first order differential
equation, which has solutions that are physically transparent. The
analysis shows that sufficiently oblique waves, propagating at
sub-ion acoustic speeds, form soliton pulse-like solutions whose
amplitudes are greatest for perpendicular propagation.  Waves that
propagate supersonically have periodic cnoidal waveforms, which are
asymmetric about the compressive and rarefactive phases of the wave.
It is also shown that there exist critical driver fields for which
the end point of the compressive phase goes sonic (in the wave
frame), with the consequence that the wave form develops a cusp. It
is possible that this trans-sonic, choked flow feature provides a
mechanism for the &quot;spiky&quot; waveforms observed in auroral electric
field measurements.</p>
</abstract>
<counts><page-count count="5"/></counts>
</article-meta>
</front>
<body/>
<back>
</back>
</article>