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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
Identificador6qtX3pFwXQZ3r59YDa/H2jMC
Repositóriosid.inpe.br/iris@1916/2005/08.01.13.56   (acesso restrito)
Última Atualização2005:08.01.03.00.00 (UTC) administrator
Repositório de Metadadossid.inpe.br/iris@1916/2005/08.01.13.56.32
Última Atualização dos Metadados2021:07.18.04.01.20 (UTC) administrator
Chave SecundáriaINPE-12914-PRE/8196
ISSN1364-6826
Chave de CitaçãoEcherAlveAlar:2005:StStMa
TítuloA statistical study of magnetic cloud parameters and geoeffectiveness
Ano2005
MêsJuly
Data de Acesso28 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho480 KiB
2. Contextualização
Autor1 Echer, Ezequiel
2 Alves, Maria Virginia
3 Alarcon, Walter Demetrio Gonzales
Identificador de Curriculo1 8JMKD3MGP5W/3C9JH3D
2 8JMKD3MGP5W/3C9JHRS
Grupo1 DGE-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espaciais
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Volume67
Número10
Páginas839-852
Histórico (UTC)2005-08-01 13:56:32 :: sergio -> administrator ::
2006-09-28 22:30:00 :: administrator -> sergio ::
2008-01-07 12:52:53 :: sergio -> administrator ::
2008-06-10 22:39:32 :: administrator -> marciana ::
2011-05-30 01:44:07 :: marciana -> administrator ::
2021-07-18 04:01:20 :: administrator -> marciana :: 2005
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-Chavemagnetic clouds
solar wind
geomagnetic storms
space weather / SOLAR-WIND
GEOMAGNETIC STORMS
INTERPLANETARY
POLARITY
ORIGIN
SIGNATURES
EVENTS
PLASMA
FIELDS
SHOCKS
ResumoA statistical study of magnetic cloud parameters and geoeffectiveness is presented in this work, based on the analysis of 149 magnetic clouds during the period 1966-2001. The distributions of maximum magnetic field strength, solar wind speed and southward magnetic field inside the clouds were determined for the whole data set and for subsets classified according to the magnetic cloud polarity (rotation in Z or Y directions). The geoeffectiveness was determined by classifying the number of magnetic clouds followed by intense, moderate and weak magnetic storms, and by calm periods. It was found that around 77% of the magnetic clouds are geoeffective, i.e., they were followed by intense or moderate geomagnetic storms (Dst <= - 50nT). Considering also weak storms (Dst <= -30nT), 97% of MCs were followed by geomagnetic activity. When considering polarity, each magnetic cloud subset has a slightly different geoeffectiveness, which is in agreement with the differences observed in their parameter distributions. The NSY_ was observed to be the less geoeffective of the MC subsets, with 66.6% of this class events being followed by intense or moderate storms, against 73.0%, of SNY+, 80.0% of the Y, 83.3% of the NSY_ and 85.7% of the SNY_. The B-peak-V-peak relation was confirmed for the magnetic clouds with rotation in Z direction. (c) 2005 Elsevier Ltd. All rights reserved. .
ÁreaCEA
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4. Condições de acesso e uso
Idiomaen
Arquivo Alvostatistical study.pdf
Grupo de Usuáriosadministrator
sergio
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/banon/2003/08.15.17.40
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
e-Mail (login)marciana
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