Formation of self-organized shear structures in thin current sheets
Self‐consistent kinetic (particle‐in‐cell) model of magnetotail thin current sheet (TCS) is used to understand the formation of self‐consistent sheared magnetic structures. It is shown that shear configurations appear in TCS as a result of self‐consistent evolution of some initial magnetic perturbat...
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Veröffentlicht in: | Journal of geophysical research. Space physics 2015-06, Vol.120 (6), p.4802-4824 |
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creator | Malova, H. V. Mingalev, O. V. Grigorenko, E. E. Mingalev, I. V. Melnik, M. N. Popov, V. Yu Delcourt, D. C. Petrukovich, A. A. Shen, C. Rong, Z. J. Zelenyi, L. M. |
description | Self‐consistent kinetic (particle‐in‐cell) model of magnetotail thin current sheet (TCS) is used to understand the formation of self‐consistent sheared magnetic structures. It is shown that shear configurations appear in TCS as a result of self‐consistent evolution of some initial magnetic perturbation at the current sheet center. Two general shapes of shear TCS components are found as a function of the transverse coordinate: symmetric and antisymmetric. We show that TCS formation goes together with the emergence of field‐aligned currents in the center of the current sheet, as a result of north‐south asymmetry of quasi‐adiabatic ion motions. Ion drift currents can also contribute to the magnetic shear evolution, but their role is much less significant, their contribution depending upon the normal component Bz and the amplitude of the initial perturbation in TCS. Parametric maps illustrating different types of TCS equilibria are presented that show a higher probability of formation of symmetric shear TCS configuration at lower values of the normal magnetic component.
Key Points
Thin current sheet model with shear magnetic component is developed
Magnetic shear can be formed self‐consistently in current sheets
Ion dynamics asymmetry in current sheets is the reason of shear appearance |
doi_str_mv | 10.1002/2014JA020974 |
format | Article |
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Key Points
Thin current sheet model with shear magnetic component is developed
Magnetic shear can be formed self‐consistently in current sheets
Ion dynamics asymmetry in current sheets is the reason of shear appearance</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1002/2014JA020974</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Astrophysics ; Asymmetry ; Configurations ; Current sheets ; Drift currents ; Evolution ; Formations ; Geophysics ; kinetic theory ; Magnetic fields ; magnetic shear ; magnetotail current sheet ; Magnetotails ; Mathematical models ; numerical modeling ; particle dynamics ; Perturbation ; Perturbation methods ; Physics ; Plasma Physics ; Shear ; Symmetry</subject><ispartof>Journal of geophysical research. Space physics, 2015-06, Vol.120 (6), p.4802-4824</ispartof><rights>2015. American Geophysical Union. All Rights Reserved.</rights><rights>Copyright Blackwell Publishing Ltd. Jun 2015</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c6518-b53863ef4113c47dc4da230ab27da868e74b1bbe7cb029eb633f310d8913794f3</citedby><cites>FETCH-LOGICAL-c6518-b53863ef4113c47dc4da230ab27da868e74b1bbe7cb029eb633f310d8913794f3</cites><orcidid>0000-0002-3103-8250</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2F2014JA020974$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2F2014JA020974$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>230,314,776,780,881,1411,1427,27901,27902,45550,45551,46384,46808</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01551999$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Malova, H. V.</creatorcontrib><creatorcontrib>Mingalev, O. V.</creatorcontrib><creatorcontrib>Grigorenko, E. E.</creatorcontrib><creatorcontrib>Mingalev, I. V.</creatorcontrib><creatorcontrib>Melnik, M. N.</creatorcontrib><creatorcontrib>Popov, V. Yu</creatorcontrib><creatorcontrib>Delcourt, D. C.</creatorcontrib><creatorcontrib>Petrukovich, A. A.</creatorcontrib><creatorcontrib>Shen, C.</creatorcontrib><creatorcontrib>Rong, Z. J.</creatorcontrib><creatorcontrib>Zelenyi, L. M.</creatorcontrib><title>Formation of self-organized shear structures in thin current sheets</title><title>Journal of geophysical research. Space physics</title><addtitle>J. Geophys. Res. Space Physics</addtitle><description>Self‐consistent kinetic (particle‐in‐cell) model of magnetotail thin current sheet (TCS) is used to understand the formation of self‐consistent sheared magnetic structures. It is shown that shear configurations appear in TCS as a result of self‐consistent evolution of some initial magnetic perturbation at the current sheet center. Two general shapes of shear TCS components are found as a function of the transverse coordinate: symmetric and antisymmetric. We show that TCS formation goes together with the emergence of field‐aligned currents in the center of the current sheet, as a result of north‐south asymmetry of quasi‐adiabatic ion motions. Ion drift currents can also contribute to the magnetic shear evolution, but their role is much less significant, their contribution depending upon the normal component Bz and the amplitude of the initial perturbation in TCS. Parametric maps illustrating different types of TCS equilibria are presented that show a higher probability of formation of symmetric shear TCS configuration at lower values of the normal magnetic component.
Key Points
Thin current sheet model with shear magnetic component is developed
Magnetic shear can be formed self‐consistently in current sheets
Ion dynamics asymmetry in current sheets is the reason of shear appearance</description><subject>Astrophysics</subject><subject>Asymmetry</subject><subject>Configurations</subject><subject>Current sheets</subject><subject>Drift currents</subject><subject>Evolution</subject><subject>Formations</subject><subject>Geophysics</subject><subject>kinetic theory</subject><subject>Magnetic fields</subject><subject>magnetic shear</subject><subject>magnetotail current sheet</subject><subject>Magnetotails</subject><subject>Mathematical models</subject><subject>numerical modeling</subject><subject>particle dynamics</subject><subject>Perturbation</subject><subject>Perturbation methods</subject><subject>Physics</subject><subject>Plasma Physics</subject><subject>Shear</subject><subject>Symmetry</subject><issn>2169-9380</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqN0c1u1DAQAOAIgUTV9sYDROICEqEzHsc_x2Vht5RVkRCUo-UkDpuSjYudQMvT41VKhXqo8MG2Rt-MNDNZ9gzhNQKwEwbIzxbAQEv-KDtgKHShObDHf_-k4Gl2HOMlpKNSCMuDbLnyYWfHzg-5b_Po-rbw4Zsdut-uyePW2ZDHMUz1OAUX827Ix2266ikEN4x74MZ4lD1pbR_d8e17mH1Zvfu8PC02H9fvl4tNUYsSVVGVpAS5liNSzWVT88YyAlsx2VgllJO8wqpysq6AaVcJopYQGqWRpOYtHWYv57pb25ur0O1suDHeduZ0sTH7GGBZotb6Jyb7YrZXwf-YXBzNrou163s7OD9FgxKVJk0g_oOmyaaqjBJ9fo9e-ikMqWnDWElEfF_zAZWmLjRDDSypV7Oqg48xuPauJQSz36j5d6OJ08x_db27edCas_WnRZq4UCmrmLO6OLrruywbvhshSZbm6_naSPjw5mL1tjQX9Aeeiayr</recordid><startdate>201506</startdate><enddate>201506</enddate><creator>Malova, H. V.</creator><creator>Mingalev, O. V.</creator><creator>Grigorenko, E. E.</creator><creator>Mingalev, I. V.</creator><creator>Melnik, M. N.</creator><creator>Popov, V. Yu</creator><creator>Delcourt, D. C.</creator><creator>Petrukovich, A. A.</creator><creator>Shen, C.</creator><creator>Rong, Z. J.</creator><creator>Zelenyi, L. M.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union/Wiley</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-3103-8250</orcidid></search><sort><creationdate>201506</creationdate><title>Formation of self-organized shear structures in thin current sheets</title><author>Malova, H. V. ; Mingalev, O. V. ; Grigorenko, E. E. ; Mingalev, I. V. ; Melnik, M. N. ; Popov, V. Yu ; Delcourt, D. C. ; Petrukovich, A. A. ; Shen, C. ; Rong, Z. J. ; Zelenyi, L. M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c6518-b53863ef4113c47dc4da230ab27da868e74b1bbe7cb029eb633f310d8913794f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Astrophysics</topic><topic>Asymmetry</topic><topic>Configurations</topic><topic>Current sheets</topic><topic>Drift currents</topic><topic>Evolution</topic><topic>Formations</topic><topic>Geophysics</topic><topic>kinetic theory</topic><topic>Magnetic fields</topic><topic>magnetic shear</topic><topic>magnetotail current sheet</topic><topic>Magnetotails</topic><topic>Mathematical models</topic><topic>numerical modeling</topic><topic>particle dynamics</topic><topic>Perturbation</topic><topic>Perturbation methods</topic><topic>Physics</topic><topic>Plasma Physics</topic><topic>Shear</topic><topic>Symmetry</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Malova, H. V.</creatorcontrib><creatorcontrib>Mingalev, O. V.</creatorcontrib><creatorcontrib>Grigorenko, E. E.</creatorcontrib><creatorcontrib>Mingalev, I. V.</creatorcontrib><creatorcontrib>Melnik, M. N.</creatorcontrib><creatorcontrib>Popov, V. Yu</creatorcontrib><creatorcontrib>Delcourt, D. C.</creatorcontrib><creatorcontrib>Petrukovich, A. A.</creatorcontrib><creatorcontrib>Shen, C.</creatorcontrib><creatorcontrib>Rong, Z. J.</creatorcontrib><creatorcontrib>Zelenyi, L. M.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Journal of geophysical research. Space physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Malova, H. V.</au><au>Mingalev, O. V.</au><au>Grigorenko, E. E.</au><au>Mingalev, I. V.</au><au>Melnik, M. N.</au><au>Popov, V. Yu</au><au>Delcourt, D. C.</au><au>Petrukovich, A. A.</au><au>Shen, C.</au><au>Rong, Z. J.</au><au>Zelenyi, L. M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Formation of self-organized shear structures in thin current sheets</atitle><jtitle>Journal of geophysical research. Space physics</jtitle><addtitle>J. Geophys. Res. Space Physics</addtitle><date>2015-06</date><risdate>2015</risdate><volume>120</volume><issue>6</issue><spage>4802</spage><epage>4824</epage><pages>4802-4824</pages><issn>2169-9380</issn><eissn>2169-9402</eissn><abstract>Self‐consistent kinetic (particle‐in‐cell) model of magnetotail thin current sheet (TCS) is used to understand the formation of self‐consistent sheared magnetic structures. It is shown that shear configurations appear in TCS as a result of self‐consistent evolution of some initial magnetic perturbation at the current sheet center. Two general shapes of shear TCS components are found as a function of the transverse coordinate: symmetric and antisymmetric. We show that TCS formation goes together with the emergence of field‐aligned currents in the center of the current sheet, as a result of north‐south asymmetry of quasi‐adiabatic ion motions. Ion drift currents can also contribute to the magnetic shear evolution, but their role is much less significant, their contribution depending upon the normal component Bz and the amplitude of the initial perturbation in TCS. Parametric maps illustrating different types of TCS equilibria are presented that show a higher probability of formation of symmetric shear TCS configuration at lower values of the normal magnetic component.
Key Points
Thin current sheet model with shear magnetic component is developed
Magnetic shear can be formed self‐consistently in current sheets
Ion dynamics asymmetry in current sheets is the reason of shear appearance</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2014JA020974</doi><tpages>23</tpages><orcidid>https://orcid.org/0000-0002-3103-8250</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Astrophysics Asymmetry Configurations Current sheets Drift currents Evolution Formations Geophysics kinetic theory Magnetic fields magnetic shear magnetotail current sheet Magnetotails Mathematical models numerical modeling particle dynamics Perturbation Perturbation methods Physics Plasma Physics Shear Symmetry |
title | Formation of self-organized shear structures in thin current sheets |
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