Local particle flux reversal under strongly sheared flow

The advection of electron density by turbulent E×B flow with linearly varying mean yields a particle flux that can reverse sign at certain locations along the direction of magnetic shear. The effect, calculated for strong flow shear, resides in the density-potential cross phase. It is produced by th...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physics of plasmas 2003-04, Vol.10 (4), p.1066-1074
Hauptverfasser: Terry, P. W., Newman, D. E., Ware, A. S.
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 1074
container_issue 4
container_start_page 1066
container_title Physics of plasmas
container_volume 10
creator Terry, P. W.
Newman, D. E.
Ware, A. S.
description The advection of electron density by turbulent E×B flow with linearly varying mean yields a particle flux that can reverse sign at certain locations along the direction of magnetic shear. The effect, calculated for strong flow shear, resides in the density-potential cross phase. It is produced by the interplay between the inhomogeneities of magnetic shear and flow shear, but subject to a variety of conditions and constraints. The regions of reversed flux tend to wash out if the turbulence consists of closely spaced modes of different helicities, but survive if modes of a single helicity are relatively isolated. The reversed flux becomes negligible if the electron density response is governed by electron scales while the eigenmode is governed by ion scales. The relationship of these results to experimentally observe flux reversals is discussed.
doi_str_mv 10.1063/1.1559475
format Article
fullrecord <record><control><sourceid>scitation_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1063_1_1559475</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>pop</sourcerecordid><originalsourceid>FETCH-LOGICAL-c297t-2ef83fb6d804b04c744bbf5d7b7cc7d4b6fbb61e358b3d0a689ac2212753c3c73</originalsourceid><addsrcrecordid>eNp9z0tLxDAUBeAgCo6jC_9Btwodk-bZpQy-oOBGwV1IbhKt1KYkndH593aYQReCq3u4fBw4CJ0TvCBY0CuyIJzXTPIDNCNY1aUUkh1us8SlEOzlGJ3k_I4xZoKrGVJNBNMVg0ljC50vQrf6KpJf-5Sn96p3PhV5TLF_7TZFfvMmeTeh-HmKjoLpsj_b3zl6vr15Wt6XzePdw_K6KaGq5VhWPigarHAKM4sZSMasDdxJKwGkY1YEawXxlCtLHTZC1QaqilSSU6Ag6Rxd7HohxZyTD3pI7YdJG02w3k7WRO8nT_ZyZzO0oxnb2P_gdUy_UA8u_If_Nn8Dz5plew</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Local particle flux reversal under strongly sheared flow</title><source>AIP Journals Complete</source><source>AIP Digital Archive</source><creator>Terry, P. W. ; Newman, D. E. ; Ware, A. S.</creator><creatorcontrib>Terry, P. W. ; Newman, D. E. ; Ware, A. S.</creatorcontrib><description>The advection of electron density by turbulent E×B flow with linearly varying mean yields a particle flux that can reverse sign at certain locations along the direction of magnetic shear. The effect, calculated for strong flow shear, resides in the density-potential cross phase. It is produced by the interplay between the inhomogeneities of magnetic shear and flow shear, but subject to a variety of conditions and constraints. The regions of reversed flux tend to wash out if the turbulence consists of closely spaced modes of different helicities, but survive if modes of a single helicity are relatively isolated. The reversed flux becomes negligible if the electron density response is governed by electron scales while the eigenmode is governed by ion scales. The relationship of these results to experimentally observe flux reversals is discussed.</description><identifier>ISSN: 1070-664X</identifier><identifier>EISSN: 1089-7674</identifier><identifier>DOI: 10.1063/1.1559475</identifier><identifier>CODEN: PHPAEN</identifier><language>eng</language><ispartof>Physics of plasmas, 2003-04, Vol.10 (4), p.1066-1074</ispartof><rights>American Institute of Physics</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c297t-2ef83fb6d804b04c744bbf5d7b7cc7d4b6fbb61e358b3d0a689ac2212753c3c73</citedby><cites>FETCH-LOGICAL-c297t-2ef83fb6d804b04c744bbf5d7b7cc7d4b6fbb61e358b3d0a689ac2212753c3c73</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/pop/article-lookup/doi/10.1063/1.1559475$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,780,784,794,1559,4512,27924,27925,76384,76390</link.rule.ids></links><search><creatorcontrib>Terry, P. W.</creatorcontrib><creatorcontrib>Newman, D. E.</creatorcontrib><creatorcontrib>Ware, A. S.</creatorcontrib><title>Local particle flux reversal under strongly sheared flow</title><title>Physics of plasmas</title><description>The advection of electron density by turbulent E×B flow with linearly varying mean yields a particle flux that can reverse sign at certain locations along the direction of magnetic shear. The effect, calculated for strong flow shear, resides in the density-potential cross phase. It is produced by the interplay between the inhomogeneities of magnetic shear and flow shear, but subject to a variety of conditions and constraints. The regions of reversed flux tend to wash out if the turbulence consists of closely spaced modes of different helicities, but survive if modes of a single helicity are relatively isolated. The reversed flux becomes negligible if the electron density response is governed by electron scales while the eigenmode is governed by ion scales. The relationship of these results to experimentally observe flux reversals is discussed.</description><issn>1070-664X</issn><issn>1089-7674</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><recordid>eNp9z0tLxDAUBeAgCo6jC_9Btwodk-bZpQy-oOBGwV1IbhKt1KYkndH593aYQReCq3u4fBw4CJ0TvCBY0CuyIJzXTPIDNCNY1aUUkh1us8SlEOzlGJ3k_I4xZoKrGVJNBNMVg0ljC50vQrf6KpJf-5Sn96p3PhV5TLF_7TZFfvMmeTeh-HmKjoLpsj_b3zl6vr15Wt6XzePdw_K6KaGq5VhWPigarHAKM4sZSMasDdxJKwGkY1YEawXxlCtLHTZC1QaqilSSU6Ag6Rxd7HohxZyTD3pI7YdJG02w3k7WRO8nT_ZyZzO0oxnb2P_gdUy_UA8u_If_Nn8Dz5plew</recordid><startdate>200304</startdate><enddate>200304</enddate><creator>Terry, P. W.</creator><creator>Newman, D. E.</creator><creator>Ware, A. S.</creator><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>200304</creationdate><title>Local particle flux reversal under strongly sheared flow</title><author>Terry, P. W. ; Newman, D. E. ; Ware, A. S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c297t-2ef83fb6d804b04c744bbf5d7b7cc7d4b6fbb61e358b3d0a689ac2212753c3c73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Terry, P. W.</creatorcontrib><creatorcontrib>Newman, D. E.</creatorcontrib><creatorcontrib>Ware, A. S.</creatorcontrib><collection>CrossRef</collection><jtitle>Physics of plasmas</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Terry, P. W.</au><au>Newman, D. E.</au><au>Ware, A. S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Local particle flux reversal under strongly sheared flow</atitle><jtitle>Physics of plasmas</jtitle><date>2003-04</date><risdate>2003</risdate><volume>10</volume><issue>4</issue><spage>1066</spage><epage>1074</epage><pages>1066-1074</pages><issn>1070-664X</issn><eissn>1089-7674</eissn><coden>PHPAEN</coden><abstract>The advection of electron density by turbulent E×B flow with linearly varying mean yields a particle flux that can reverse sign at certain locations along the direction of magnetic shear. The effect, calculated for strong flow shear, resides in the density-potential cross phase. It is produced by the interplay between the inhomogeneities of magnetic shear and flow shear, but subject to a variety of conditions and constraints. The regions of reversed flux tend to wash out if the turbulence consists of closely spaced modes of different helicities, but survive if modes of a single helicity are relatively isolated. The reversed flux becomes negligible if the electron density response is governed by electron scales while the eigenmode is governed by ion scales. The relationship of these results to experimentally observe flux reversals is discussed.</abstract><doi>10.1063/1.1559475</doi><tpages>9</tpages></addata></record>
fulltext fulltext
identifier ISSN: 1070-664X
ispartof Physics of plasmas, 2003-04, Vol.10 (4), p.1066-1074
issn 1070-664X
1089-7674
language eng
recordid cdi_crossref_primary_10_1063_1_1559475
source AIP Journals Complete; AIP Digital Archive
title Local particle flux reversal under strongly sheared flow
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-21T03%3A52%3A30IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-scitation_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Local%20particle%20flux%20reversal%20under%20strongly%20sheared%20flow&rft.jtitle=Physics%20of%20plasmas&rft.au=Terry,%20P.%20W.&rft.date=2003-04&rft.volume=10&rft.issue=4&rft.spage=1066&rft.epage=1074&rft.pages=1066-1074&rft.issn=1070-664X&rft.eissn=1089-7674&rft.coden=PHPAEN&rft_id=info:doi/10.1063/1.1559475&rft_dat=%3Cscitation_cross%3Epop%3C/scitation_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true