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Metadados

1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3Q9K2TS
Repositóriosid.inpe.br/mtc-m21b/2017/12.27.15.04
Última Atualização2021:02.19.12.33.27 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21b/2017/12.27.15.04.30
Última Atualização dos Metadados2022:03.18.22.12.27 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoJauerAPPVASS:2017:StMaFi
TítuloStudy of magnetic field spatial variations in the southern hemisphere's low latitudes due to different interplanetary structures using the 3-D MHD SWMF/BATSRUS model
Ano2017
Data de Acesso04 jun. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho73 KiB
2. Contextualização
Autor1 Jauer, Paulo Ricardo
2 Alves, Livia Ribeiro
3 Padilha, Antônio Lopes
4 Pádua, Marcelo Banik de
5 Vitorello, Ícaro
6 Alves, Maria Virginia
7 Silva, Ligia Alves da
8 Souza, Vitor Moura Cardoso e Silva
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JGJG
4 8JMKD3MGP5W/3C9JHNR
5 8JMKD3MGP5W/3C9JHD6
6 8JMKD3MGP5W/3C9JHRS
Grupo1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
5 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
6 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
7 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
8 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
8 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 paulo.jauer@inpe.br
2 livia.alves@inpe.br
3 antonio.padilha@inpe.br
4 marcelo.banik@inpe.br
5
6 ma.alves@inpe.br
7 ligia.silva@inpe.br
Nome do EventoAGU Fall Meeting
Localização do EventoNew Orleans
Data11-15 Dec.
Título do LivroProceedings
Histórico (UTC)2017-12-27 15:04:30 :: simone -> administrator ::
2018-06-04 02:28:10 :: administrator -> simone :: 2017
2021-02-19 12:33:27 :: simone -> administrator :: 2017
2022-03-18 22:12:27 :: administrator -> simone :: 2017
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
ResumoInterplanetary structures such as Coronal Mass Ejections (CME), Shocks, Corotating Interaction Regions (CIR) and Magnetic Clouds (MC) interfere directly on Space Weather conditions and can cause severe and intense disturbances in the Earth's magnetic field as measured in space and on the ground. During magnetically disturbed periods characterized by world-wide, abrupt variations of the geomagnetic field, large and intense current systems can be induced and amplified within the Earth even at low latitudes. Such current systems are known as geomagnetically induced currents (GIC) and can cause damage to power transmission lines, transformers and the degradation of pipelines. As part of an effort to estimate GIC intensities throughout the low to equatorial latitudes of the Brazilian territory, we used the 3-D MHD SWMF/BATSRUS code to estimate spatial variations of the geomagnetic field during periods when the magnetosphere is under the influence of CME and MC structures. Specifically, we used the CalcDeltaB tool (Rastatter et al., Space Weather, 2014) to provide a proxy for the spatial variations of the geomagnetic field, with a 1 minute cadence, at 31 virtual magnetometer stations located in the proposed study region. The stations are spatially arranged in a two-dimensional network with each station being 5 degrees apart in latitude and longitude. In a preliminary analysis, we found that prior to the arrival of each interplanetary structure, there is no appreciable variation in the components of the geomagnetic field between the virtual stations. However, when the interplanetary structures reach the magnetosphere, each station perceives the magnetic field variation differently, so that it is not possible to use a single station to represent the magnetic field perturbation throughout the Brazilian region. We discuss the minimum number and spacing between stations to adequately detail the geomagnetic field variations in this region.
ÁreaCEA
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 27/12/2017 13:04 1.0 KiB 
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34P/3Q9K2TS
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34P/3Q9K2TS
Idiomaen
Arquivo Alvojauer_study.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhosid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.55.54 2
sid.inpe.br/mtc-m21/2012/07.13.14.40.26 2
sid.inpe.br/mtc-m21/2012/07.13.14.54.32 1
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url volume
7. Controle da descrição
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