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<article language="en">
	<journal>
		<journal_title>Astrophysics and Space Sciences Transactions</journal_title>
		<journal_url>www.astrophys-space-sci-trans.net</journal_url>
		<issn>1810-6528</issn>
		<eissn>1810-6536</eissn>
		<volume_number>4</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/astra-4-35-2008</doi>
	<article_url>http://www.astrophys-space-sci-trans.net/4/35/2008/</article_url>
	<abstract_html>http://www.astrophys-space-sci-trans.net/4/35/2008/astra-4-35-2008.html</abstract_html>
	<fulltext_pdf>http://www.astrophys-space-sci-trans.net/4/35/2008/astra-4-35-2008.pdf</fulltext_pdf>
	<start_page>35</start_page>
	<end_page>40</end_page>
	<publication_date>2008-07-08</publication_date>
	<article_title content_type="html">Magnetic turbulence in and around the Earth&apos;s magnetosphere</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>G. Zimbardo</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>A. Greco</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>P. Veltri</name>
		</author>
		<author numeration="4" affiliations="2,4">
			<name>Z. Voros</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>A. L. Taktakishvili</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">University of Calabria, Department of Physics, Rende, Italy</affiliation>
		<affiliation numeration="2" content_type="html">Institute of Atmospheric Research, Prague, Czech Republic</affiliation>
		<affiliation numeration="3" content_type="html">Tbilisi State University, Tbilisi, Georgia</affiliation>
		<affiliation numeration="4" content_type="html">also at: Institute of Astro- and Particle Physics, University  of Innsbruck, Austria</affiliation>
	</affiliations>
	<abstract content_type="html">Magnetic turbulence is found in most space plasmas, including the geospace
environment. Recent spacecraft observations
of magnetic turbulence in the ion foreshock,
in the magnetosheath, in the polar cusp regions, and in the magnetotail
will be reviewed. Turbulence features like the fluctuation level, the
spectral power law index, the turbulence anisotropy and intermittency, and
the turbulence driver will be addressed.
The influence of such a turbulence on the plasma
transport and dynamics will be described, also using the results of
numerical simulations.</abstract>
	<references>
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</article>
