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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZGivnJVY/Lraor
Repositóriosid.inpe.br/mtc-m16@80/2006/06.12.14.29
Última Atualização2015:06.10.19.05.29 (UTC) seeger05
Repositório de Metadadossid.inpe.br/mtc-m16@80/2006/06.12.14.29.15
Última Atualização dos Metadados2024:05.15.10.57.15 (UTC) seeger05
Chave SecundáriaINPE--PRE/
ISSN1808-0804
Rótuloself-archiving-INPE-MCTI-GOV-BR
Chave de CitaçãoNishinoMaYuMiScAb:2006:EnPaPr
TítuloEnergetic particle precipitation in The Brazilian geomagnetic anomaly during the "Bastille Day Storm" of July 2000
Ano2006
MêsMay
Data de Acesso22 jun. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PN
Número de Arquivos1
Tamanho3995 KiB
2. Contextualização
Autor1 Nishino, Masanori
2 Makita, Kazuo
3 Yumoto, Kiyofumi
4 Miyoshi, Yoshizumi
5 Schuh, Nelson J.
6 Abdu, Mangalathayil Ali
Grupo1
2
3
4
5 RSU-INPE-MCT-BR
6 DAE-INPE-MCT-BR
Afiliação1 Nagoya University
2 Takushoku University
3 Kyushu University
4 Nagoya University
5 Soutrher Space REsearch Center, Rio Grande do Sul (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 stel nishino@yahoo.co.jp 
2  
3  
4  
5 njschuch@lacesm.ufsm.br 
6 abdu@dae.inpe.br
RevistaEarth, Planets and Space
Volume58
Número5
Páginas607-616
Histórico (UTC)2006-06-12 17:50:06 :: seeger05 -> marciana ::
2006-08-03 16:40:33 :: marciana -> administrator ::
2006-09-28 22:32:40 :: administrator -> seeger05 ::
2006-12-04 19:39:23 :: seeger05 -> administrator ::
2008-06-10 22:42:24 :: administrator -> banon ::
2010-05-11 15:35:16 :: banon -> administrator ::
2013-10-09 08:27:14 :: administrator -> seeger05 :: 2006
2015-06-10 19:05:30 :: seeger05 -> administrator :: 2006
2021-07-28 22:48:31 :: administrator -> seeger05 :: 2006
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-ChaveBastille Day Storm
Brazilian geomagnetic anomaly
energetic particle precipitation
imaging riometer
ResumoIonospheric absorption associated with a great geomagnetic storm on July 15-16, 2000 (the "Bastille Day storm") was observed in the Brazilian geomagnetic anomaly using a two-dimensional 4×4 imaging riometer (IRIS). In the afternoon of July 15, weak absorption (~0.2 dB) was observed during the initial phase of the storm; large spatial-scale absorption exceeded the IRIS field of view (330×330 km). During the sharp magnetic decrease in the main phase of the storm, absorption was intensified (<0.5 dB) in the evening, showing a sheet structure with ~150 km latitudinal width and >330 km longitudinal elongation. Subsequently, absorption was intensified (~1 dB), having a small spatial-scale (~150 km) in the background sheet structure and a pronounced westward drift (~570 m s-1). In association with large magnetic fluctuations in the Bz component of the interplanetary magnetic field (IMF), the ground magnetic variation in the night sector showed large positive swings during the initial to main phases of the storm. With the subsequent southward turning of the IMF Bz, the ground magnetic variation in the evening sector showed rapid storm development. Particle fluxes measured by a geosynchronous satellite (L = ~6.6) demonstrated large enhancements of low-energy protons (50-400 keV) and probably electrons (50-225 keV) during the storm's initial phase. Particle fluxes from the low-altitude NOAA satellite (~870 km) indicated the invasion of low-energy particles into the region of L < 2 during the main phase of the storm. These results indicate that low-energy particles injected into the outer radiation belt in association with frequent and strong substorm occurrences, were transported into the inner radiation belt through direct convective access by the storm-induced electric fields during the storm's development. These particles then precipitated into the ionosphere over the Brazilian geomagnetic anomaly. Notably, the most intense absorption could be dominantly caused by proton precipitation with energies of ~40 keV. Key words: Bastille Day storm, Brazilian geomagnetic anomaly, energetic particle precipitation, imaging riometer.
ÁreaCEA
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Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/6qtX3pFwXQZGivnJVY/Lraor
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZGivnJVY/Lraor
Idiomaen
Arquivo Alvonishino_energetic.pdf
Grupo de Usuáriosadministrator
banon
seeger05
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.04.21.53 1
DivulgaçãoPORTALCAPES
Acervo Hospedeirosid.inpe.br/banon/2003/08.15.17.40
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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