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<article language="en">
	<journal>
		<journal_title>Nonlinear Processes  in Geophysics</journal_title>
		<journal_url>www.nonlin-processes-geophys.net</journal_url>
		<issn>1023-5809</issn>
		<eissn>1607-7946</eissn>
		<volume_number>9</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/npg-9-87-2002</doi>
	<article_url>http://www.nonlin-processes-geophys.net/9/87/2002/</article_url>
	<abstract_html>http://www.nonlin-processes-geophys.net/9/87/2002/npg-9-87-2002.html</abstract_html>
	<fulltext_pdf>http://www.nonlin-processes-geophys.net/9/87/2002/npg-9-87-2002.pdf</fulltext_pdf>
	<start_page>87</start_page>
	<end_page>99</end_page>
	<publication_date>0000-00-00</publication_date>
	<article_title content_type="html">Nonlinear waves and solitons propagating perpendicular to the magnetic field in bi-ion plasma with finite plasma pressure</article_title>
	<authors>
		<author numeration="1" affiliations="1,3">
			<name>E. M. Dubinin</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>K. Sauer</name>
		</author>
		<author numeration="3" affiliations="1,2">
			<name>J. F. McKenzie</name>
		</author>
		<author numeration="4" affiliations="3">
			<name>G. Chanteur</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max-Planck Institut für Aeronomie, Katlenburg-Lindau, Germany</affiliation>
		<affiliation numeration="2" content_type="html">School of Pure and Applied Physics, University of Natal, Durban, South Africa</affiliation>
		<affiliation numeration="3" content_type="html">Centre d’Etude des Environnements Terrestre et Planetaires, Velizy, France</affiliation>
	</affiliations>
	<abstract content_type="html">We investigate the
      nature of nonlinear waves propagating transverse to the magnetic field in
      a bi-ion plasma including plasma pressure. By using the conservation laws
      derived from the multi-ion fluid equations the system may be described by
      a single order differential equation whose properties control the
      structure of the flow and the magnetic field. Compressive solitons exist
      in specific ranges of the characteristic Mach numbers. Various features of
      solitons differ in different existence &amp;quot;windows&amp;quot;. For example,
      there are solitons that contain a strong proton rarefaction core embedded
      in the main compressional structure. Compressive solitons are found in a
      wide range of flow parameters. Finite ion pressure introduces critical
      Mach numbers. In contrast to a plasma consisting only of protons and
      electrons these singular points are reached where a specific combination
      of ion and electron speeds lies on particular locii, in multi-parameter
      space, which corresponds to the generalized &amp;quot;sonic point&amp;quot; of the
      compound system.</abstract>
	<references>
	</references>
</article>

