1. Identificação | |
Tipo de Referência | Artigo em Evento (Conference Proceedings) |
Site | mtc-m21b.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34P/3Q9K2TS |
Repositório | sid.inpe.br/mtc-m21b/2017/12.27.15.04 |
Última Atualização | 2021:02.19.12.33.27 (UTC) simone |
Repositório de Metadados | sid.inpe.br/mtc-m21b/2017/12.27.15.04.30 |
Última Atualização dos Metadados | 2022:03.18.22.12.27 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
Chave de Citação | JauerAPPVASS:2017:StMaFi |
Título | Study 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 |
Ano | 2017 |
Data de Acesso | 23 set. 2024 |
Tipo Secundário | PRE CI |
Número de Arquivos | 1 |
Tamanho | 73 KiB |
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2. Contextualização | |
Autor | 1 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 Curriculo | 1 2 3 8JMKD3MGP5W/3C9JGJG 4 8JMKD3MGP5W/3C9JHNR 5 8JMKD3MGP5W/3C9JHD6 6 8JMKD3MGP5W/3C9JHRS |
Grupo | 1 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 |
Afiliação | 1 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 Autor | 1 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 Evento | AGU Fall Meeting |
Localização do Evento | New Orleans |
Data | 11-15 Dec. |
Título do Livro | Proceedings |
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 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Tipo de Versão | publisher |
Resumo | Interplanetary 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. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Study of magnetic... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Study of magnetic... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
URL dos dados | http://urlib.net/ibi/8JMKD3MGP3W34P/3Q9K2TS |
URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP3W34P/3Q9K2TS |
Idioma | en |
Arquivo Alvo | jauer_study.pdf |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Repositório Espelho | sid.inpe.br/mtc-m21b/2013/09.26.14.25.22 |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3F2PBEE |
Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.40.26 9 sid.inpe.br/mtc-m21/2012/07.13.14.55.54 6 sid.inpe.br/bibdigital/2013/10.12.21.02 4 |
Acervo Hospedeiro | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notas | |
Campos Vazios | archivingpolicy 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 |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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