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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositóriosid.inpe.br/mtc-m17@80/2007/11.27.12.36
Repositório de Metadadossid.inpe.br/mtc-m17@80/2007/11.27.12.36.47
Última Atualização dos Metadados2018:06.05.03.35.30 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoEcherAlvGonBalGua:2007:GeInVa
TítuloGeomagnetic index variability and ring current asymmetry during april 1999 (magnetic cloud driven) and february 2000 (complex ejecta driven)
Ano2007
Data de Acesso21 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Echer, Ezequiel
2 Alves, Maria Virgínia
3 Gonzalez Alarcon, Walter Demétrio
4 Balmaceda, Laura A.
5 Guarnieri, Fernando Luís
Grupo1 DGE-INPE-MCT-BR
2 LAP-INPE-MCT-BR
3 DGE-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Max Planck Institute fuer Sonnensystemforschung
5 UNIVAP
Nome do EventoEuropean Geosciences Union General Assembly 2007 (EGU Assembly).
Localização do EventoVienna, Austria
Data15-20 Apr.
Título do LivroProceedings
Tipo TerciárioOral Session
Histórico (UTC)2007-11-27 12:36:47 :: simone -> administrator ::
2012-10-24 00:03:13 :: administrator -> simone ::
2013-02-20 15:20:08 :: simone -> administrator :: 2007
2018-06-05 03:35:30 :: administrator -> marciana :: 2007
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoThere are basically two types of interplanetary ejecta: magnetic clouds (MC) and complex ejecta (CE). In this work we present a comparison of the geomagnetic activity during two magnetic storms associated with different interplanetary ejecta. The first magnetic storm was observed on April 16-17, 1999, and it was driven by a MC; it shows a smooth and regular storm development. The other event, observed on February 11-13, 2000, was caused by the interaction of two interplanetary coronal mass ejections and shocks (complex ejecta). Observations of this CE show a very irregular and fluctuating storm development. The behavior of the geomagnetic activity during these two different storms is analyzed by using the Kp and Dst indices. Further, the ring current asymmetry is investigated through the SYM-H and ASY-H high resolution indices and ground-based observations of low latitude magnetometers. This study is a continuation of our previous works that have analyzed solar and interplanetary events of these two Sun-Earth connection events.
ÁreaCEA
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4. Condições de acesso e uso
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Grupo de Usuáriosadministrator
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Visibilidadeshown
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ET2RFS
8JMKD3MGPCW/3EU29DP
Acervo Hospedeirolcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark type url versiontype volume
7. Controle da descrição
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