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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-14-373-2007</article-id>
<title-group>
<article-title>Magnetic holes in plasmas close to the mirror instability</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Borgogno</surname>
<given-names>D.</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>Passot</surname>
<given-names>T.</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>Sulem</surname>
<given-names>P. L.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>CNRS, Observatoire de la C&amp;#x00D4;te d&apos;Azur, B.P. 4229, 06304 Nice Cedex 4, France</addr-line>
</aff>
<pub-date pub-type="epub">
<day>09</day>
<month>07</month>
<year>2007</year>
</pub-date>
<volume>14</volume>
<issue>4</issue>
<fpage>373</fpage>
<lpage>383</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2007 D. Borgogno et al.</copyright-statement>
<copyright-year>2007</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/14/373/2007/npg-14-373-2007.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/14/373/2007/npg-14-373-2007.pdf</self-uri>
<abstract>
<p>Non-propagating magnetic hole solutions in anisotropic plasmas near
the mirror instability threshold are investigated in numerical
simulations of a fluid model that incorporates linear Landau damping
and finite Larmor radius corrections calculated in the gyrokinetic
approximation. This FLR-Landau fluid model reproduces
the subcritical mirror bifurcation recently identified on the
Vlasov-Maxwell system, both by theory and numerics.
Stable magnetic hole solutions that display a polarization
different from that of Hall-MHD solitons are indeed obtained slighlty
below threshold, while magnetic patterns and spatio-temporal chaos emerge when
the system is maintained in a mirror unstable regime.</p>
</abstract>
<counts><page-count count="11"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>