1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | mtc-m21b.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34P/3J4BUGL |
Repositório | sid.inpe.br/mtc-m21b/2015/03.04.19.33 |
Última Atualização | 2015:03.04.19.33.09 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/mtc-m21b/2015/03.04.19.33.09 |
Última Atualização dos Metadados | 2018:06.04.02.55.17 (UTC) administrator |
DOI | 10.1088/0004-637X/799/1/39 |
ISSN | 0004-637X 1538-4357 |
Chave de Citação | HajraTsuEchGonSan:2015:ReE>0. |
Título | Relativistic (E> 0.6, > 2.0, and > 4.0 MeV) elelctron acceleration at geosynchronous orbit during high-intensity, long-duration, continuous AE activity (HILDCAA) events |
Ano | 2015 |
Data de Acesso | 08 maio 2024 |
Tipo de Trabalho | journal article |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 1272 KiB |
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2. Contextualização | |
Autor | 1 Hajra, Rajkumar 2 Tsurutani, Bruce T. 3 Echer, Ezequiel 4 Gonzalez Alarcon, Walter Demétrio 5 Santolik, Ondrei |
Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JH3D 4 8JMKD3MGP5W/3C9JJC4 |
Grupo | 1 DGE-CEA-INPE-MCTI-GOV-BR 2 3 DGE-CEA-INPE-MCTI-GOV-BR 4 DGE-CEA-INPE-MCTI-GOV-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) |
Endereço de e-Mail do Autor | 1 rajkumarhajra@yahoo.co.in 2 3 eecher@dge.inpe.br 4 gonzalez@dge.inpe.br |
Revista | Astrophysical Journal |
Volume | 799 |
Número | 1 |
Nota Secundária | A1_ASTRONOMIA_/_FÍSICA A1_QUÍMICA A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_INTERDISCIPLINAR A2_ENGENHARIAS_IV B2_ENSINO |
Histórico (UTC) | 2015-03-04 19:33:09 :: simone -> administrator :: 2018-06-04 02:55:17 :: administrator -> simone :: 2015 |
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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 |
Palavras-Chave | acceleration of particles magnetic reconnection relativistic processes solar wind waves |
Resumo | Radiation-belt relativistic (E > 0.6, > 2.0, and > 4.0 MeV) electron acceleration is studied for solar cycle 23 (1995-2008). High-intensity, long-duration, continuous AE activity (HILDCAA) events are considered as the basis of the analyses. All of the 35 HILDCAA events under study were found to be characterized by flux enhancements of magnetospheric relativistic electrons of all three energies compared to the pre-event flux levels. For the E > 2.0 MeV electron fluxes, enhancement of > 50% occurred during 100% of HILDCAAs. Cluster-4 passes were examined for electromagnetic chorus waves in the 5 < L < 10 and 0 < MLT < 12 region when wave data were available. Fully 100% of these HILDCAA cases were associated with enhanced whistler-mode chorus waves. The enhancements of E > 0.6, > 2.0, and > 4.0 MeV electrons occurred similar to 1.0 day, similar to 1.5 days, and similar to 2.5 days after the statistical HILDCAA onset, respectively. The statistical acceleration rates for the three energy ranges were similar to 1.8 x 10(5), 2.2 x 10(3), and 1.0 x 10(1) cm(-2) s(-1) sr(-1) d(-1), respectively. The relativistic electron-decay timescales were determined to be similar to 7.7, 5.5, and 4.0 days for the three energy ranges, respectively. The HILDCAAs were divided into short-duration (D <= 3 days) and long-duration (D > 3 days) events to study the dependence of relativistic electron variation on HILDCAA duration. For long-duration events, the flux enhancements during HILDCAAs with respect to pre-event fluxes were similar to 290%, 520%, and 82% for E > 0.6, > 2.0, and > 4.0 MeV electrons, respectively. The enhancements were similar to 250%, 400%, and 27% respectively, for short-duration events. The results are discussed with respect to the current understanding of radiation-belt dynamics. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Relativistic (E> 0.6,... |
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/3J4BUGL |
URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP3W34P/3J4BUGL |
Idioma | en |
Arquivo Alvo | Hajra_relativistic.pdf |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Política de Arquivamento | allowpublisher allowfinaldraft |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Repositório Espelho | urlib.net/www/2011/03.29.20.55 |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.15.01.50 4 sid.inpe.br/mtc-m21/2012/07.13.14.45.47 3 sid.inpe.br/bibdigital/2013/10.01.22.11 1 |
Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. |
Acervo Hospedeiro | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark month nextedition notes orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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