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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/44CTBEL
Repositóriosid.inpe.br/mtc-m21c/2021/03.24.12.03
Repositório de Metadadossid.inpe.br/mtc-m21c/2021/03.24.12.03.18
Última Atualização dos Metadados2022:04.03.19.25.08 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoMirandaChiaHuMunõ:2021:MuCrCo
TítuloMultifractality and cross-scale coupling in interplanetary magnetic field turbulence during a rope-rope magnetic reconnection event
Ano2021
Data de Acesso13 maio 2024
Tipo SecundárioPRE CN
2. Contextualização
Autor1 Miranda, R. A.
2 Chian, Abraham Chian-Long
3 Hu, Q.
4 Munõz, P. R.
Grupo1
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Universidade de Brasília (UnB)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 University of Alabama in Huntsville
4 University of La Serena
Nome do EventoSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA)
Localização do EventoOnline
Data22-26 mar.
Histórico (UTC)2021-03-24 12:03:18 :: simone -> administrator ::
2022-04-03 19:25:08 :: administrator -> simone :: 2021
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoWe analyze the multifractal scaling of the modulus of the magnetic field |B| during a rope-rope magnetic reconnection event measured by ACE and Cluster on 1 February 2002. This event is characterized by three interplanetary magnetic flux ropes (IMFR), a bifurcated current sheet, and evidence of rope-rope magnetic reconnection. The time series of |B| is divided into five intervals corresponding to interior regions and boundary layers of the three IMFRs. We quantify the degree of intermittency by computing the scaling exponents of the structure functions at each interval, and show that the magnetic reconnection occurring in the interface between two flux ropes can act as a source of intermittent magnetic field turbulence. We also analyze the relation between the skewness and the kurtosis, and demonstrate that the parabolic relation displays scale dependence and is enhanced during magnetic reconnection. These results indicate that a direct coupling between the scales of magnetic flux ropes and the scales within the inertial subrange occurs in the solar wind.
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5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/46KTFK8
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
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