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Charged particle acceleration by intermittent electromagnetic turbulence
We studied the role of intermittency in the process of acceleration and transport of charged particles by electromagnetic turbulence. We propose a simple model of electromagnetic turbulence with a variable level of intermittency. The magnetic field is described as a superposition of an ensemble of m...
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Published in: | Geophysical research letters 2011-09, Vol.38 (17), p.n/a |
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creator | Zelenyi, L. M. Rybalko, S. D. Artemyev, A. V. Petrukovich, A. A. Zimbardo, G. |
description | We studied the role of intermittency in the process of acceleration and transport of charged particles by electromagnetic turbulence. We propose a simple model of electromagnetic turbulence with a variable level of intermittency. The magnetic field is described as a superposition of an ensemble of magnetostatic plane waves and of spatially localized dynamic magnetic clouds. The amplitudes of magnetic clouds are distributed according to an intermittent map. The model approximates essential properties of turbulence observed ‘in situ’ in the neutral plane of the Earth's magnetotail. Numerical integration of charged particle trajectories in such a dynamic electromagnetic environment shows that, for the fixed time interval, the higher the level of intermittency, the higher the energy gain. Moreover, in a sufficiently intermittent turbulence, particle acceleration occurs without significant intensification of the spatial transport.
Key Points
Model of turbulence with regulated level of intermittency is developed
The model approximates the properties of the turbulence observed in magnetotail
In intermittent turbulence acceleration occurs w/o intensification of transport |
doi_str_mv | 10.1029/2011GL048983 |
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Key Points
Model of turbulence with regulated level of intermittency is developed
The model approximates the properties of the turbulence observed in magnetotail
In intermittent turbulence acceleration occurs w/o intensification of transport</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2011GL048983</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Acceleration ; Atmospheric sciences ; Charged particles ; Computational fluid dynamics ; Earth Sciences ; Fluid flow ; Geophysics ; Intermittency ; Magnetic fields ; Magnetism ; magnetotail ; Mathematical models ; Nonlinear systems ; Physics ; Plasma physics ; Sciences of the Universe ; Space ; Space Physics ; Turbulence ; Turbulent flow ; turbulent transport and acceleration</subject><ispartof>Geophysical research letters, 2011-09, Vol.38 (17), p.n/a</ispartof><rights>Copyright 2011 by the American Geophysical Union.</rights><rights>Copyright 2011 by American Geophysical Union</rights><rights>Attribution</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c5097-420c1e69401c0dac64bfe8c9ef333dd1d4cdebfba23f02a2c15d6ca3e94056553</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2011GL048983$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2011GL048983$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>230,314,780,784,885,11513,27923,27924,46467,46891</link.rule.ids><backlink>$$Uhttps://hal.science/hal-00655044$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Zelenyi, L. M.</creatorcontrib><creatorcontrib>Rybalko, S. D.</creatorcontrib><creatorcontrib>Artemyev, A. V.</creatorcontrib><creatorcontrib>Petrukovich, A. A.</creatorcontrib><creatorcontrib>Zimbardo, G.</creatorcontrib><title>Charged particle acceleration by intermittent electromagnetic turbulence</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>We studied the role of intermittency in the process of acceleration and transport of charged particles by electromagnetic turbulence. We propose a simple model of electromagnetic turbulence with a variable level of intermittency. The magnetic field is described as a superposition of an ensemble of magnetostatic plane waves and of spatially localized dynamic magnetic clouds. The amplitudes of magnetic clouds are distributed according to an intermittent map. The model approximates essential properties of turbulence observed ‘in situ’ in the neutral plane of the Earth's magnetotail. Numerical integration of charged particle trajectories in such a dynamic electromagnetic environment shows that, for the fixed time interval, the higher the level of intermittency, the higher the energy gain. Moreover, in a sufficiently intermittent turbulence, particle acceleration occurs without significant intensification of the spatial transport.
Key Points
Model of turbulence with regulated level of intermittency is developed
The model approximates the properties of the turbulence observed in magnetotail
In intermittent turbulence acceleration occurs w/o intensification of transport</description><subject>Acceleration</subject><subject>Atmospheric sciences</subject><subject>Charged particles</subject><subject>Computational fluid dynamics</subject><subject>Earth Sciences</subject><subject>Fluid flow</subject><subject>Geophysics</subject><subject>Intermittency</subject><subject>Magnetic fields</subject><subject>Magnetism</subject><subject>magnetotail</subject><subject>Mathematical models</subject><subject>Nonlinear systems</subject><subject>Physics</subject><subject>Plasma physics</subject><subject>Sciences of the Universe</subject><subject>Space</subject><subject>Space Physics</subject><subject>Turbulence</subject><subject>Turbulent flow</subject><subject>turbulent transport and acceleration</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp9kU1P20AQhldVkUihN36A1UvLwTD7Ya_3GEUlQTJBQi3htlqvx7DUsdP1Gsi_70apItRDTzOaed5X80HIGYULCkxdMqB0XoIoVME_kAlVQqQFgPxIJgAq5kzmx-TTMDwDAAdOJ2QxezL-EetkY3xwtsXEWIstehNc3yXVNnFdQL92IWAXktixwfdr89hhxJMw-mpssbN4So4a0w74-W88IT-vvv-YLdLydn49m5apzUDJVDCwFHMlgFqojc1F1WBhFTac87qmtbA1Vk1lGG-AGWZpVufWcIyKLM8yfkLO975PptUb79bGb3VvnF5MS72rAUQMhHihkf26Zze-_z3iEPTaDXG71nTYj4NWlCkWL7dz_fZfkkopqVC54hH98g_63I--iztrFa1kRnMRIbaHXl2L28OcFPTuUfr9o_T8rmSFUDKK0r3IDQHfDiLjf-lccpnp1XKuH-5Xy1VW3ugl_wO5opXj</recordid><startdate>201109</startdate><enddate>201109</enddate><creator>Zelenyi, L. 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M. ; Rybalko, S. D. ; Artemyev, A. V. ; Petrukovich, A. A. ; Zimbardo, G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5097-420c1e69401c0dac64bfe8c9ef333dd1d4cdebfba23f02a2c15d6ca3e94056553</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Acceleration</topic><topic>Atmospheric sciences</topic><topic>Charged particles</topic><topic>Computational fluid dynamics</topic><topic>Earth Sciences</topic><topic>Fluid flow</topic><topic>Geophysics</topic><topic>Intermittency</topic><topic>Magnetic fields</topic><topic>Magnetism</topic><topic>magnetotail</topic><topic>Mathematical models</topic><topic>Nonlinear systems</topic><topic>Physics</topic><topic>Plasma physics</topic><topic>Sciences of the Universe</topic><topic>Space</topic><topic>Space Physics</topic><topic>Turbulence</topic><topic>Turbulent flow</topic><topic>turbulent transport and acceleration</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zelenyi, L. 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M.</au><au>Rybalko, S. D.</au><au>Artemyev, A. V.</au><au>Petrukovich, A. A.</au><au>Zimbardo, G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Charged particle acceleration by intermittent electromagnetic turbulence</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2011-09</date><risdate>2011</risdate><volume>38</volume><issue>17</issue><epage>n/a</epage><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>We studied the role of intermittency in the process of acceleration and transport of charged particles by electromagnetic turbulence. We propose a simple model of electromagnetic turbulence with a variable level of intermittency. The magnetic field is described as a superposition of an ensemble of magnetostatic plane waves and of spatially localized dynamic magnetic clouds. The amplitudes of magnetic clouds are distributed according to an intermittent map. The model approximates essential properties of turbulence observed ‘in situ’ in the neutral plane of the Earth's magnetotail. Numerical integration of charged particle trajectories in such a dynamic electromagnetic environment shows that, for the fixed time interval, the higher the level of intermittency, the higher the energy gain. Moreover, in a sufficiently intermittent turbulence, particle acceleration occurs without significant intensification of the spatial transport.
Key Points
Model of turbulence with regulated level of intermittency is developed
The model approximates the properties of the turbulence observed in magnetotail
In intermittent turbulence acceleration occurs w/o intensification of transport</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2011GL048983</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Acceleration Atmospheric sciences Charged particles Computational fluid dynamics Earth Sciences Fluid flow Geophysics Intermittency Magnetic fields Magnetism magnetotail Mathematical models Nonlinear systems Physics Plasma physics Sciences of the Universe Space Space Physics Turbulence Turbulent flow turbulent transport and acceleration |
title | Charged particle acceleration by intermittent electromagnetic turbulence |
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