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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/45D52JB
Repositóriosid.inpe.br/mtc-m21d/2021/09.07.15.24
Última Atualização2021:09.07.15.24.34 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21d/2021/09.07.15.24.34
Última Atualização dos Metadados2022:04.03.19.24.01 (UTC) administrator
DOI10.1029/2021JA029363
ISSN2169-9402
Chave de CitaçãoSilvaSASMMVACSDJWLLAS:2021:StAn
TítuloHigh-Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to the Alfvénic Fluctuations Within High-Speed Solar Wind Stream: A Statistical Analysis
Ano2021
MêsAug.
Data de Acesso06 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho9474 KiB
2. Contextualização
Autor 1 Silva, Ligia Alves da
 2 Shi, J.
 3 Alves, Livia Ribeiro
 4 Sibeck, D.
 5 Marchezi, José Paulo
 6 Medeiros, Cláudia
 7 Vieira, Luís Eduardo Antunes
 8 Agapitov, O.
 9 Cardoso, F. R.
10 Souza, Vitor Moura Cardoso e Silva
11 Dal Lago, Alisson
12 Jauer, Paulo Roberto
13 Wang, C.
14 Li, H.
15 Liu, Z.
16 Alves, Maria Virgínia
17 Silva, Marlos Rockenbach da
Identificador de Curriculo 1
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11 8JMKD3MGP5W/3C9JGH3
12
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16 8JMKD3MGP5W/3C9JHRS
ORCID 1 0000-0002-8822-5030
 2 0000-0002-8008-0527
 3 0000-0002-5680-7271
 4 0000-0003-3240-7510
 5 0000-0002-2904-6411
 6 0000-0002-6914-5799
 7 0000-0002-9376-475X
 8 0000-0001-6427-1596
 9 0000-0001-7239-0894
10 0000-0001-7294-7963
11 0000-0002-4361-6492
12 0000-0002-8064-5030
13 0000-0001-6991-9398
14 0000-0002-4839-4614
15 0000-0001-8034-5575
16 0000-0002-7477-1233
17 0000-0002-9737-9429
Grupo 1 DIHPA-CGCE-INPE-MCTI-GOV-BR
 2
 3 DIHPA-CGCE-INPE-MCTI-GOV-BR
 4
 5 DIHPA-CGCE-INPE-MCTI-GOV-BR
 6 DIHPA-CGCE-INPE-MCTI-GOV-BR
 7 DIHPA-CGCE-INPE-MCTI-GOV-BR
 8
 9
10 DIHPA-CGCE-INPE-MCTI-GOV-BR
11 DIHPA-CGCE-INPE-MCTI-GOV-BR
12 DIHPA-CGCE-INPE-MCTI-GOV-BR
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16 DIHPA-CGCE-INPE-MCTI-GOV-BR
17 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Chinese Academy of Sciences
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 NASA Goddard Space Flight Center
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 University of California
 9 Universidade de São Paulo (USP)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Chinese Academy of Sciences
14 Chinese Academy of Sciences
15 Chinese Academy of Sciences
16 Instituto Nacional de Pesquisas Espaciais (INPE)
17 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor 1 ligia.alves01@gmail.com
RevistaJournal of Geophysical Research: Space Physics
Volume126
Número8
Páginase2021JA029363
Histórico (UTC)2021-09-07 15:24:34 :: simone -> administrator ::
2021-09-07 15:24:35 :: administrator -> simone :: 2021
2021-09-07 15:30:32 :: simone -> administrator :: 2021
2022-04-03 19:24:01 :: administrator -> simone :: 2021
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chaveelectron flux enhancement
high speed solar wind stream
high-energy electron flux
outer radiation belt
ultra low frequency waves
whistler-mode chorus waves
ResumoThe coupling response between solar wind structures and the magnetosphere is highly complex, leading to different effects in the outer radiation belt electron fluxes. Most Coronal Mass Ejections cause strong geomagnetic storms with short recovery phases, often 12 days. By contrast, High-Speed Solar Wind Streams lead to moderate and weak storms often with much longer recovery phases, from several to ∼10 days. The magnetosphere receives energy for a long time under the influence of the HSSs, considerably changing its dynamics. This in turn has an effect on the charged particles trapped in the outer radiation belt. Although the high-energy electron flux enhancements have received considerable attention, the high-energy electron flux enhancement pattern (L > 4) has not. This paper identifies 37 events with this enhancement pattern in the high-energy electron flux during the Van Allen Probes era. We find the enhancements coincident with HSS occurrence. The interplanetary magnetic field (IMF) exhibits north/south Bz fluctuations of Alfvénic nature with moderate amplitudes. The high-energy electron flux enhancements also correspond to long periods of auroral activity indicating a relationship to magnetotail dynamics. However, the AE index only reaches moderate values. Ultra-Low Frequency waves were present in all of the events and whistler-mode chorus waves were present in 89.1% of the events, providing a convenient scenario for wave-particle interactions. The radial gradient of the ULF wave power related to the L, under the influence of the HSSs, is necessary to trigger the physical processes responsible for this type of high-energy electron flux enhancement pattern.
ÁreaCEA
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34T/45D52JB
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34T/45D52JB
Idiomaen
Arquivo Alvosilva_high.pdf
Grupo de Usuáriossimone
Visibilidadeshown
Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/46KTFK8
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.39.46 2
sid.inpe.br/mtc-m21/2012/07.13.14.55.54 2
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirourlib.net/www/2021/06.04.03.40
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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