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Plasmoids Formation During Simulations of Coaxial Helicity Injection in the National Spherical Torus Experiment
The formation of an elongated Sweet-Parker current sheet and a transition to plasmoid instability has for the first time been predicted by simulations in a large-scale toroidal fusion plasma in the absence of any preexisting instability. Plasmoid instability is demonstrated through resistive MHD sim...
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Published in: | Physical review letters 2015-05, Vol.114 (20), p.205003-205003, Article 205003 |
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description | The formation of an elongated Sweet-Parker current sheet and a transition to plasmoid instability has for the first time been predicted by simulations in a large-scale toroidal fusion plasma in the absence of any preexisting instability. Plasmoid instability is demonstrated through resistive MHD simulations of transient coaxial helicity injection experiments in the National Spherical Torus Experiment (NSTX). Consistent with the theory, fundamental characteristics of the plasmoid instability, including fast reconnection rate, have been observed in these realistic simulations. Motivated by the simulations, experimental camera images have been revisited and suggest the existence of reconnecting plasmoids in NSTX. Global, system-size plasmoid formation observed here should also have strong implications for astrophysical reconnection, such as rapid eruptive solar events. |
doi_str_mv | 10.1103/physrevlett.114.205003 |
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Plasmoid instability is demonstrated through resistive MHD simulations of transient coaxial helicity injection experiments in the National Spherical Torus Experiment (NSTX). Consistent with the theory, fundamental characteristics of the plasmoid instability, including fast reconnection rate, have been observed in these realistic simulations. Motivated by the simulations, experimental camera images have been revisited and suggest the existence of reconnecting plasmoids in NSTX. 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Global, system-size plasmoid formation observed here should also have strong implications for astrophysical reconnection, such as rapid eruptive solar events.</description><subject>Current sheets</subject><subject>Elongation</subject><subject>Formations</subject><subject>Helicity</subject><subject>Instability</subject><subject>Plasmoids</subject><subject>Simulation</subject><subject>Stability</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqFkUFP3DAQha2KqmwpfwFZnLiEztiJ4z2iLRSkVYsKnC3HsVmjJA6xg9h_j9mlvfZk--l7nnl6hJwgnCMC_z5utnGyL51NKQvlOYMKgH8iC4R6WdRZOiCLrGCxBKgPydcYnwAAmZBfyCETUNaMVwsSbjsd--DbSK_C1Ovkw0B_zJMfHumd7-dup0QaHF0F_ep1R69t541PW3ozPFmzM_iBpo2lv3ZwRu7GjZ28ybf7MM2RXr6O-d3bIX0jn53uoj3-OI_Iw9Xl_eq6WP_-ebO6WBem4jIVzNbScmZKAMFdjiFa57AB40qx1LJxjRaNyBFa5kQLDTfIqtqJ0qCUrGL8iJzu_w0xeRXzvtZsTBiGvLFClKzk79DZHhqn8DzbmFTvo7Fdpwcb5qiwlgIlgIT_o0KKEhErzKjYo2YKMZfk1Jiz62mrENR7eeo2l_fHvqxzeVko1b68bDz5mDE3vW3_2f62xd8A4oaZAg</recordid><startdate>20150520</startdate><enddate>20150520</enddate><creator>Ebrahimi, F</creator><creator>Raman, R</creator><general>American Physical Society</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20150520</creationdate><title>Plasmoids Formation During Simulations of Coaxial Helicity Injection in the National Spherical Torus Experiment</title><author>Ebrahimi, F ; Raman, R</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c538t-2e78e32c40063f0316dff1b0cf469a8bfba6b6723d2f6d0b3c1257f64c1882523</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Current sheets</topic><topic>Elongation</topic><topic>Formations</topic><topic>Helicity</topic><topic>Instability</topic><topic>Plasmoids</topic><topic>Simulation</topic><topic>Stability</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ebrahimi, F</creatorcontrib><creatorcontrib>Raman, R</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ebrahimi, F</au><au>Raman, R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Plasmoids Formation During Simulations of Coaxial Helicity Injection in the National Spherical Torus Experiment</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2015-05-20</date><risdate>2015</risdate><volume>114</volume><issue>20</issue><spage>205003</spage><epage>205003</epage><pages>205003-205003</pages><artnum>205003</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>The formation of an elongated Sweet-Parker current sheet and a transition to plasmoid instability has for the first time been predicted by simulations in a large-scale toroidal fusion plasma in the absence of any preexisting instability. 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source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Current sheets Elongation Formations Helicity Instability Plasmoids Simulation Stability |
title | Plasmoids Formation During Simulations of Coaxial Helicity Injection in the National Spherical Torus Experiment |
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