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	<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>16</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/npg-16-631-2009</doi>
	<article_url>http://www.nonlin-processes-geophys.net/16/631/2009/</article_url>
	<abstract_html>http://www.nonlin-processes-geophys.net/16/631/2009/npg-16-631-2009.html</abstract_html>
	<fulltext_pdf>http://www.nonlin-processes-geophys.net/16/631/2009/npg-16-631-2009.pdf</fulltext_pdf>
	<start_page>631</start_page>
	<end_page>639</end_page>
	<publication_date>2009-11-04</publication_date>
	<article_title content_type="html">Acceleration and transport of ions in turbulent current sheets: formation of non-maxwelian energy distribution</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>A. V. Artemyev</name>
			<email>ante0226@gmail.com</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>L. M. Zelenyi</name>
		</author>
		<author numeration="3" affiliations="1,2">
			<name>H. V. Malova</name>
		</author>
		<author numeration="4" affiliations="3">
			<name>G. Zimbardo</name>
		</author>
		<author numeration="5" affiliations="4">
			<name>D. Delcourt</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Space Research Institute, RAS, Profsoyusnaya Street 84/32, Moscow, Russia</affiliation>
		<affiliation numeration="2" content_type="html">Nuclear Physics Institute, Moscow State University, Moscow, Russia</affiliation>
		<affiliation numeration="3" content_type="html">Dipartimento di Fisica, Universita della Calabria, 87036 Arcavacatadi Rende, Italy</affiliation>
		<affiliation numeration="4" content_type="html">Laboratoire de Physique des Plasmas, CNRS, Saint-Maur-des-FossÃ©s, France</affiliation>
	</affiliations>
	<abstract content_type="html">The paper is devoted to particle acceleration in turbulent current sheet
(CS). Our results show that the mechanism of CS particle interaction with
electromagnetic turbulence can explain the formation of power law energy
distributions. We study the ratio between adiabatic acceleration of particles
in electric field in the presence of stationary turbulence and acceleration
due to electric field in the case of dynamic turbulence. The correlation
between average energy gained by particles and average particle residence
time in the vicinity of the neutral sheet is discussed. It is also
demonstrated that particle velocity distributions formed by
particle-turbulence interaction are similar in essence to the ones observed
near the far reconnection region in the Earth&apos;s magnetotail.</abstract>
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</article>

