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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>14</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/npg-14-351-2007</doi>
	<article_url>http://www.nonlin-processes-geophys.net/14/351/2007/</article_url>
	<abstract_html>http://www.nonlin-processes-geophys.net/14/351/2007/npg-14-351-2007.html</abstract_html>
	<fulltext_pdf>http://www.nonlin-processes-geophys.net/14/351/2007/npg-14-351-2007.pdf</fulltext_pdf>
	<start_page>351</start_page>
	<end_page>359</end_page>
	<publication_date>2007-07-06</publication_date>
	<article_title content_type="html">Three-dimensional simulations of turbulent spectra in the local interstellar medium</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>D. Shaikh</name>
			<email>dastgeer@ucr.edu</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>G. P. Zank</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Geophysics and Planetary Physics, University of  California, Riverside CA 92521, USA</affiliation>
	</affiliations>
	<abstract content_type="html">Three-dimensional time dependent numerical simulations of compressible
magnetohydrodynamic fluids describing super-Alfvénic, supersonic and
strongly magnetized space and laboratory plasmas show a nonlinear
relaxation towards a state of near incompressibility. The latter is
characterized essentially by a subsonic turbulent Mach number.  This
transition is mediated dynamically by disparate spectral energy
dissipation rates in compressible magnetosonic and shear Alfvénic
modes. Nonlinear cascades lead to super-Alfvénic turbulent motions
decaying to a sub-Alfvénic regime that couples weakly with
(magneto)acoustic cascades. Consequently, the supersonic plasma motion
is transformed into highly subsonic motion and density fluctuations
experience a passive convection. This model provides a self-consistent
explaination of the ubiquitous nature of incompressible magnetoplasma
fluctuations in the solar wind and the interstellar medium.</abstract>
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</article>

