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<!DOCTYPE article SYSTEM "http://www.nonlin-processes-geophys.net/inc/npg/copernicus.dtd">
<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>5/6</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/npg-9-487-2002</doi>
	<article_url>http://www.nonlin-processes-geophys.net/9/487/2002/</article_url>
	<abstract_html>http://www.nonlin-processes-geophys.net/9/487/2002/npg-9-487-2002.html</abstract_html>
	<fulltext_pdf>http://www.nonlin-processes-geophys.net/9/487/2002/npg-9-487-2002.pdf</fulltext_pdf>
	<start_page>487</start_page>
	<end_page>496</end_page>
	<publication_date>0000-00-00</publication_date>
	<article_title content_type="html">Baroclinic instability of a symmetric, rotating, stratified flow: a study of the nonlinear stabilisation mechanisms in the presence of viscosity</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>R. Mantovani</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>A. Speranza</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Mathematics Department, University of Camerino, Via Madonna delle Carceri, 62032 Camerino (MC), Italy</affiliation>
		<affiliation numeration="2" content_type="html">presently: ESRIN, European Space Agency, Via Galileo Galilei, 00044 Frascati, Italy</affiliation>
	</affiliations>
	<abstract content_type="html">This paper presents
      the analysis of symmetric circulations of a rotating baroclinic flow,
      forced by a steady thermal wind and dissipated by Laplacian friction. The
      analysis is performed with numerical time-integration. Symmetric flows,
      vertically bound by horizontal walls and subject to either periodic or
      vertical wall lateral boundary conditions, are investigated in the region
      of parameter-space where unstable small amplitude modes evolve into stable
      stationary nonlinear solutions. The distribution of solutions in
      parameter-space is analysed up to the threshold of chaotic behaviour and
      the physical nature of the nonlinear interaction operating on the finite
      amplitude unstable modes is investigated. In particular, analysis of
      time-dependent energy-conversions allows understanding of the physical
      mechanisms operating from the initial phase of linear instability to the
      finite amplitude stable state. Vertical shear of the basic flow is shown
      to play a direct role in injecting energy into symmetric flow since the
      stage of linear growth. Dissipation proves essential not only in limiting
      the energy of linearly unstable modes, but also in selecting their
      dominant space-scales in the finite amplitude stage.</abstract>
	<references>
	</references>
</article>

