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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3P8SECKy/CUcBP
Repositóriosid.inpe.br/jeferson/2004/07.28.14.25   (acesso restrito)
Última Atualização2006:06.14.04.10.08 (UTC) administrator
Repositório de Metadadossid.inpe.br/jeferson/2004/07.28.14.25.27
Última Atualização dos Metadados2021:07.18.04.01.46 (UTC) administrator
Chave SecundáriaINPE-11205-PRE/6654
ISSN1364-6826
Chave de CitaçãoTsurutaniGoGuKaZhAr:2004:ArHiLo
TítuloAre high-intensity long-duration continuous AE activity (HILDCAA) events substorm expansion events?
Ano2004
Data de Acesso04 maio 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho994 KiB
2. Contextualização
Autor1 Tsurutani, Bruce T.
2 Gonzalez-Alarcon, Walte Demetrio
3 Guarnieri, Fernando
4 Kamidec, Yosuke
5 Zhoua, Xiaoyan
6 Arballoa, John K.
Grupo1 DGE-INPE-MCT-BR
Afiliação1 Jet Propulsion Laboratory, California Institute of Technology
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Solar-Terrestrial Environment Laboratory, Nagoya University
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Volume66
Páginas167-176
Histórico (UTC)2006-01-18 18:35:07 :: marciana -> administrator ::
2007-03-09 22:20:04 :: administrator -> marciana ::
2008-05-02 16:20:26 :: marciana -> administrator ::
2021-07-18 04:01:46 :: administrator -> marciana :: 2004
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveHigh speed solar wind streams
Alfv
en waves
HILDCAAs
Substorms
ResumoHigh-intensity, long-duration, continuous AE activity (HILDCAA) are magnetospheric/ionospheric events that occur during high-speed solar wind streams. The AE increases are caused by intermittent magnetic reconnection between southward components of interplanetary Alfv;en wave <uctuations and magnetopause magnetic =elds. During solar minimum, corotating interaction regions (CIRs) created by corotating stream interactions with slow-speed streams cause relatively short duration moderate to minor magnetic storms. These storms are followed by lengthy (days to weeks) of HILDCAA intervals characterized by low levels of enhanced ring current activity (DST). Shorter HILDCAA intervals are also noted following interplanetary coronal mass ejections (ICME)-related storm events. Two intervals were chosen to study in detail using POLAR UVI imaging data to identify substorms. The =rst was an interval not associated with a storm. The second was a short interval following an ICME-related magnetic storm. Although substorms were detected during the HILDCAA intervals, there was little or no relationship between substorm occurrences and AE (−AL) increases. One possible explanation is that prompt penetration of interplanetary electric =elds associated with magnetic reconnection lead to enhanced ionospheric westward electrojet current densities (-AL increases). These same dawn-to-dusk electric =elds could lead to the convection of nightside outer magnetospheric/plasmasheet plasma, causing particle injection and DST decreases. Substorms must be caused by other processes, such as self-organized criticality.
ÁreaCEA
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4. Condições de acesso e uso
Idiomaen
Arquivo AlvoAre high-intensity.pdf
Grupo de Usuáriosadministrator
alexandra
marciana
Visibilidadeshown
Detentor da CópiaSID/SCD
Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
DivulgaçãoWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
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