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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-21-339-2014</article-id>
<title-group>
<article-title>Ion acceleration by parallel propagating nonlinear Alfvén wave packets in a radially expanding plasma</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Nariyuki</surname>
<given-names>Y.</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>Umeda</surname>
<given-names>T.</given-names>
<ext-link>https://orcid.org/0000-0001-6882-9200</ext-link>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Suzuki</surname>
<given-names>T. 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>Hada</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Faculty of Human Development, University of Toyama, 3190, Toyama City, Toyama 930-8555, Japan</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8601, Japan</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Physics, Nagoya University, Furo-cho, Nagoya, Aichi 464-8602, Japan</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Department of Earth System Science and Technology, Kyushu University, 6-1, Kasuga City, Fukuoka 816-8580, Japan</addr-line>
</aff>
<pub-date pub-type="epub">
<day>27</day>
<month>02</month>
<year>2014</year>
</pub-date>
<volume>21</volume>
<issue>1</issue>
<fpage>339</fpage>
<lpage>346</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2014 Y. Nariyuki et al.</copyright-statement>
<copyright-year>2014</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://npg.copernicus.org/articles/21/339/2014/npg-21-339-2014.html">This article is available from https://npg.copernicus.org/articles/21/339/2014/npg-21-339-2014.html</self-uri>
<self-uri xlink:href="https://npg.copernicus.org/articles/21/339/2014/npg-21-339-2014.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/21/339/2014/npg-21-339-2014.pdf</self-uri>
<abstract>
<p>The numerical simulation of the nonlinear evolution of the parallel
propagating Alfvén waves in a radially expanding plasma is performed by
using a kinetic-fluid model (the Vlasov–MHD model). In our study, both the
nonlinear evolution of the Alfvén waves and the radial evolution of the
velocity distribution function (VDF) are treated simultaneously. On the other
hand, important ion kinetic effects such as ion cyclotron damping and
instabilities driven by the non-equilibrium ion velocity distributions are
not included in the present model. The results indicate that the steepened
Alfvén wave packets outwardly accelerate ions, which can be observed as the
beam components in the interplanetary space. The energy of imposed Alfvén
waves is converted into the longitudinal fluctuations by the nonlinear
steepening and the nonlinear Landau damping. The wave shoaling due to the
inhomogeneity of the phase velocity is also observed.</p>
</abstract>
<counts><page-count count="8"/></counts>
</article-meta>
</front>
<body/>
<back>
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