Nonlinear Electromagnetic Stabilization of Plasma Microturbulence

The physical causes for the strong stabilizing effect of finite plasma β on ion-temperature-gradient-driven turbulence, which far exceeds quasilinear estimates, are identified from nonlinear gyrokinetic simulations. The primary contribution stems from a resonance of frequencies in the dominant nonli...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review letters 2018-04, Vol.120 (17), p.175002-175002, Article 175002
Hauptverfasser: Whelan, G G, Pueschel, M J, Terry, P W
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 175002
container_issue 17
container_start_page 175002
container_title Physical review letters
container_volume 120
creator Whelan, G G
Pueschel, M J
Terry, P W
description The physical causes for the strong stabilizing effect of finite plasma β on ion-temperature-gradient-driven turbulence, which far exceeds quasilinear estimates, are identified from nonlinear gyrokinetic simulations. The primary contribution stems from a resonance of frequencies in the dominant nonlinear interaction between the unstable mode, the stable mode, and zonal flows, which maximizes the triplet correlation time and therefore the energy transfer efficiency. A modification to mixing-length transport estimates is constructed, which reproduces nonlinear heat fluxes throughout the examined β range.
doi_str_mv 10.1103/physrevlett.120.175002
format Article
fullrecord <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1434991</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2038706687</sourcerecordid><originalsourceid>FETCH-LOGICAL-c533t-5104d8bf1eb79588585f49107292aebf248b997557805b8b89bbf33bb9d7fe7f3</originalsourceid><addsrcrecordid>eNpdkU1vVSEQhonR2Gv1LzQnunFzKgOHAyybpn4kV9u0uibABUvDgStwmrS_XsytLlxNMnlm8s48CJ0APgXA9MP-9qEWdx9da6dAepMzjMkztAHM5cgBpudogzGFUWLMj9CrWu8wxkBm8RIdEcnZLCjfoLNvOcWQnC7DRXS2lbzon8m1YIebpk2I4VG3kNOQ_XAVdV308DXYkttazBpdsu41euF1rO7NUz1GPz5efD__PG4vP305P9uOllHaRgZ42gnjwRkumRBMMD_JnpZIop3xZBJG9liMC8yMMEIa4yk1Ru64d9zTY_T2sDfXFlS1oTl7a3NKPbWCiU5SQofeH6B9yb9WV5taQrUuRp1cXqsimAqO51nwjr77D73La0n9BEUABBcU5Nyp-UD1m2v_uFf7EhZdHhRg9ceEuuomrt39tptQ3YQ6mOiDJ0_rV7O43b-xv6-nvwGE3Iai</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2118783196</pqid></control><display><type>article</type><title>Nonlinear Electromagnetic Stabilization of Plasma Microturbulence</title><source>American Physical Society Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><creator>Whelan, G G ; Pueschel, M J ; Terry, P W</creator><creatorcontrib>Whelan, G G ; Pueschel, M J ; Terry, P W</creatorcontrib><description>The physical causes for the strong stabilizing effect of finite plasma β on ion-temperature-gradient-driven turbulence, which far exceeds quasilinear estimates, are identified from nonlinear gyrokinetic simulations. The primary contribution stems from a resonance of frequencies in the dominant nonlinear interaction between the unstable mode, the stable mode, and zonal flows, which maximizes the triplet correlation time and therefore the energy transfer efficiency. A modification to mixing-length transport estimates is constructed, which reproduces nonlinear heat fluxes throughout the examined β range.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/physrevlett.120.175002</identifier><identifier>PMID: 29756837</identifier><language>eng</language><publisher>United States: American Physical Society</publisher><subject>Energy transfer ; Fluid dynamics ; Heat flux</subject><ispartof>Physical review letters, 2018-04, Vol.120 (17), p.175002-175002, Article 175002</ispartof><rights>Copyright American Physical Society Apr 27, 2018</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c533t-5104d8bf1eb79588585f49107292aebf248b997557805b8b89bbf33bb9d7fe7f3</citedby><cites>FETCH-LOGICAL-c533t-5104d8bf1eb79588585f49107292aebf248b997557805b8b89bbf33bb9d7fe7f3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,315,782,786,887,2878,2879,27931,27932</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/29756837$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/1434991$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Whelan, G G</creatorcontrib><creatorcontrib>Pueschel, M J</creatorcontrib><creatorcontrib>Terry, P W</creatorcontrib><title>Nonlinear Electromagnetic Stabilization of Plasma Microturbulence</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>The physical causes for the strong stabilizing effect of finite plasma β on ion-temperature-gradient-driven turbulence, which far exceeds quasilinear estimates, are identified from nonlinear gyrokinetic simulations. The primary contribution stems from a resonance of frequencies in the dominant nonlinear interaction between the unstable mode, the stable mode, and zonal flows, which maximizes the triplet correlation time and therefore the energy transfer efficiency. A modification to mixing-length transport estimates is constructed, which reproduces nonlinear heat fluxes throughout the examined β range.</description><subject>Energy transfer</subject><subject>Fluid dynamics</subject><subject>Heat flux</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNpdkU1vVSEQhonR2Gv1LzQnunFzKgOHAyybpn4kV9u0uibABUvDgStwmrS_XsytLlxNMnlm8s48CJ0APgXA9MP-9qEWdx9da6dAepMzjMkztAHM5cgBpudogzGFUWLMj9CrWu8wxkBm8RIdEcnZLCjfoLNvOcWQnC7DRXS2lbzon8m1YIebpk2I4VG3kNOQ_XAVdV308DXYkttazBpdsu41euF1rO7NUz1GPz5efD__PG4vP305P9uOllHaRgZ42gnjwRkumRBMMD_JnpZIop3xZBJG9liMC8yMMEIa4yk1Ru64d9zTY_T2sDfXFlS1oTl7a3NKPbWCiU5SQofeH6B9yb9WV5taQrUuRp1cXqsimAqO51nwjr77D73La0n9BEUABBcU5Nyp-UD1m2v_uFf7EhZdHhRg9ceEuuomrt39tptQ3YQ6mOiDJ0_rV7O43b-xv6-nvwGE3Iai</recordid><startdate>20180427</startdate><enddate>20180427</enddate><creator>Whelan, G G</creator><creator>Pueschel, M J</creator><creator>Terry, P W</creator><general>American Physical Society</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7X8</scope><scope>OTOTI</scope></search><sort><creationdate>20180427</creationdate><title>Nonlinear Electromagnetic Stabilization of Plasma Microturbulence</title><author>Whelan, G G ; Pueschel, M J ; Terry, P W</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c533t-5104d8bf1eb79588585f49107292aebf248b997557805b8b89bbf33bb9d7fe7f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Energy transfer</topic><topic>Fluid dynamics</topic><topic>Heat flux</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Whelan, G G</creatorcontrib><creatorcontrib>Pueschel, M J</creatorcontrib><creatorcontrib>Terry, P W</creatorcontrib><collection>PubMed</collection><collection>CrossRef</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>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Whelan, G G</au><au>Pueschel, M J</au><au>Terry, P W</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Nonlinear Electromagnetic Stabilization of Plasma Microturbulence</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2018-04-27</date><risdate>2018</risdate><volume>120</volume><issue>17</issue><spage>175002</spage><epage>175002</epage><pages>175002-175002</pages><artnum>175002</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>The physical causes for the strong stabilizing effect of finite plasma β on ion-temperature-gradient-driven turbulence, which far exceeds quasilinear estimates, are identified from nonlinear gyrokinetic simulations. The primary contribution stems from a resonance of frequencies in the dominant nonlinear interaction between the unstable mode, the stable mode, and zonal flows, which maximizes the triplet correlation time and therefore the energy transfer efficiency. A modification to mixing-length transport estimates is constructed, which reproduces nonlinear heat fluxes throughout the examined β range.</abstract><cop>United States</cop><pub>American Physical Society</pub><pmid>29756837</pmid><doi>10.1103/physrevlett.120.175002</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0031-9007
ispartof Physical review letters, 2018-04, Vol.120 (17), p.175002-175002, Article 175002
issn 0031-9007
1079-7114
language eng
recordid cdi_osti_scitechconnect_1434991
source American Physical Society Journals; EZB-FREE-00999 freely available EZB journals
subjects Energy transfer
Fluid dynamics
Heat flux
title Nonlinear Electromagnetic Stabilization of Plasma Microturbulence
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-03T21%3A48%3A02IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Nonlinear%20Electromagnetic%20Stabilization%20of%20Plasma%20Microturbulence&rft.jtitle=Physical%20review%20letters&rft.au=Whelan,%20G%20G&rft.date=2018-04-27&rft.volume=120&rft.issue=17&rft.spage=175002&rft.epage=175002&rft.pages=175002-175002&rft.artnum=175002&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/physrevlett.120.175002&rft_dat=%3Cproquest_osti_%3E2038706687%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2118783196&rft_id=info:pmid/29756837&rfr_iscdi=true