Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3AS39U5
Repositorysid.inpe.br/mtc-m19/2011/11.25.13.17   (restricted access)
Last Update2011:12.26.17.19.40 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/11.25.13.17.57
Metadata Last Update2018:06.05.04.25.04 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1088/2041-8205/735/1/L9
ISSN2041-8205
2041-8213
Citation KeyRempelChiaBran:2011:LaCoSt
TitleLagrangian coherent structures in nonlinear dynamos
Year2011
MonthJuly
Access Date2024, May 04
Secondary TypePRE PI
Number of Files1
Size2454 KiB
2. Context
Author1 Rempel, E. L.
2 Chian, A. C. L.
3 Brandenburg, A.
Group1
2 DGE-CEA-INPE-MCT-BR
Affiliation1 Institute of Aeronautical Technology (ITA)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 NORDITA, AlbaNova University Ctr, Stockholm, Sweden
Author e-Mail Address1 rempel@ita.br
2 abraham.chian@gmail.com
3 brandenb@nordita.org
e-Mail Addresstereza@sid.inpe.br
JournalAstrophysical Journal Letters
Volume735
Number1
PagesL9
History (UTC)2011-12-08 16:24:27 :: tereza@sid.inpe.br -> marciana :: 2011
2011-12-26 17:19:49 :: marciana -> administrator :: 2011
2018-06-05 04:25:04 :: administrator -> marciana :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordschaos
dynamo
magnetohydrodynamics (MHD
AbstractTurbulence and chaos play a fundamental role in stellar convective zones through the transport of particles, energy, and momentum, and in fast dynamos, through the stretching, twisting, and folding of magnetic flux tubes. A particularly revealing way to describe turbulent motions is through the analysis of Lagrangian coherent structures (LCSs), which are material lines or surfaces that act as transport barriers in the fluid. We report the detection of LCSs in helical MHD dynamo simulations with scale separation. In an Arnold-Beltrami-Childress flow, two dynamo regimes, a propagating coherent mean-field regime and an intermittent regime, are identified as the magnetic diffusivity is varied. The sharp contrast between the chaotic tangle of attracting and repelling LCSs in both regimes permits a unique analysis of the impact of the magnetic field on the velocity field. In a second example, LCSs reveal the link between the level of chaotic mixing of the velocity field and the saturation of a large-scale dynamo when the magnetic field exceeds the equipartition value.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Lagrangian coherent structures...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 25/11/2011 11:17 1.0 KiB 
4. Conditions of access and use
Languageen
User Groupadministrator
tereza@sid.inpe.br
marciana
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
update 


Close