Fechar

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3P8SECKy/EpUcH
Repositóriosid.inpe.br/jeferson/2004/12.09.14.22   (acesso restrito)
Última Atualização2006:06.14.04.17.00 (UTC) administrator
Repositório de Metadadossid.inpe.br/jeferson/2004/12.09.14.22.57
Última Atualização dos Metadados2021:07.18.04.01.46 (UTC) administrator
Chave SecundáriaINPE-10988-PRE/6444
ISSN1364-6826
Chave de CitaçãoEcherGGPVDGS:2004:LoTeCo
TítuloLong term correlation between solar and geomagnetic activity
Ano2004
MêsMar.
Data de Acesso04 maio 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho285 KiB
2. Contextualização
Autor1 Echer, Ezequiel
2 Gonzalez, Walter Demetrio
3 Gonzalez, Alicia Luisa Clua de
4 Prestes, A.
5 Vieira, Luis Eduardo A.
6 Dal Lago, Alisson
7 Guarnieri, Fernando Luis
8 Schuch, Nelson Jorge
Identificador de Curriculo1 8JMKD3MGP5W/3C9JH3D
2 8JMKD3MGP5W/3C9JJC4
3
4
5
6 8JMKD3MGP5W/3C9JGH3
7
8 8JMKD3MGP5W/3C9JHUD
Grupo1 DGE-INPE-MCT-BR
2 RSU-INPE-MCT-BR
3
4
5
6
7
8
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Volume66
Número12
Páginas1019-1025
Histórico (UTC)2004-12-09 16:22:58 :: alexandra -> marciana ::
2006-06-06 14:40:25 :: marciana -> administrator ::
2007-03-09 22:30:03 :: administrator -> marciana ::
2008-05-02 16:20:27 :: 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-ChaveGeomagnetic activity
Solar activity
Solar wind
Sunspot number
ResumoA long-term correlation study between solar and geomagnetic activity is reported in this work using annual averages of the aa index and of the sunspot number Rz in the period of 1868?2000. Dst and AE geomagnetic indices and solar wind speed data are used for more recent periods. It is shown that the geomagnetic and solar activity correlation has decreased since the end of the 19th century, and the lag between them has increased. The variations of Rz and aa were in phase in the early period (solar cycles 11?14, around 1868?1910), and became out of phase in later periods (with a lag of 2 years in solar cycle 22, with aa maximum after Rz). Nevertheless, this trend is not monotonic and superposed <uctuations are seen, which does not permit determine if this correlation decrease is part or not of a long period solar activity cycle. The probable cause of the correlation decrease seems to be related to the aa index dual peak structure. The second aa peak seems to have increased relative to the =rst one. This second peak is more related to the high-speed streams originated from co-rotating structures whereas the =rst one is related to sunspot (coronal mass ejections) activity. In recent periods, since 1964, it has been observed that aa annual values have higher correlation with the fraction of days per year with daily solar wind speed peaks larger than 500 km=s (Fpk) than with Rz . The aa index also shows larger correlation with AE index than with Dst. Thus, it seems that average aa is strongly in<uenced by AE activity, which is in<uenced mainly by high speed streams from coronal holes. One can conclude that the decrease in correlation between aa and Rz occurs because the second aa peak has becoming stronger relative to the =rst one. The cause seems to be that open solar magnetic =eld structures have increased their activity relative to the closed (sunspot-related) solar magnetic =eld structures. This implies that the global solar magnetic =eld could have experienced a di?erential (between closed and open structures) large-scale variation in the last 130 years. c 2004 Elsevier Ltd. All rights reserved.
ÁreaCEA
Arranjo 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Long term correlation...
Arranjo 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Long term correlation...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Arquivo Alvosdarticle.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
8JMKD3MGPCW/3EUFCFP
DivulgaçãoWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notas
Campos Vaziosaffiliation alternatejournal 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
atualizar 


Fechar