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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
Identificador6qtX3pFwXQZQjxQKY/Gt3nx
Repositóriosid.inpe.br/ePrint@80/2005/06.15.12.31   (acesso restrito)
Última Atualização2005:06.15.12.31.15 (UTC) administrator
Repositório de Metadadossid.inpe.br/ePrint@80/2005/06.15.12.31.16
Última Atualização dos Metadados2018:06.04.04.12.43 (UTC) administrator
Chave SecundáriaINPE-12559-PRE/7856
ISSN0103-9733
Chave de CitaçãoBalmacedaGESVDGG:2004:SoOrSu
TítuloThe solar origins of the Sun-Earth connection events on april 1999 and february 2000
Ano2004
Data Secundária2004
MêsDec.
Data de Acesso18 abr. 2024
Tipo SecundárioPRE PN
Número de Arquivos1
Tamanho302 KiB
2. Contextualização
Autor1 Balmaceda, L. A.
2 Gonzales Alarcon, Walter Demétrio
3 Echer, Ezequiel
4 Santos, J. C.
5 Vieira, Luis Eduardo Antunes
6 Dal Lago, Alisson
7 Guarnieri, Fernando Luiz
8 Gonzalez, Alicia Luisa Clua de
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JH3D
4
5
6 8JMKD3MGP5W/3C9JGH3
Grupo1 DGE-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial(INPE, DGE)
2 Max Planck Inst Sonnensyst Forsch
RevistaBrazilian Journal of Physics
Volume34
Número4b
Páginas1745-1747
Histórico (UTC)2010-05-14 01:58:01 :: alexandra -> administrator ::
2018-06-04 04:12:43 :: administrator -> marciana :: 2004
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoIn this work we present a comparison between the solar origins of two solar-terrestrial connection events occurring on April 1999 and February 2000, respectively. On April 13 (1999), a coronal mass ejection (CME) appeared for the first time in LASCO-C2 coronagraph field of view at 03:30 UT. The possible solar disc source of this CME was located at coordinates N25 E05, and it consisted on flaring activity together with a filament eruption as seen in EIT images. The geomagnetic storm with a Dst peak of -91 nT registered on April, 17 was attributed to this solar surface activity. On February 8, 9 and 10 (2000) three Earth-directed halo CMEs were recorded by LASCO coronagraphs. The interaction of two of them caused the intense interplanetary geomagnetic storm registered on February 12 (Dst = -110 nT). The CMEs detected on February 8 and 10 were launched from AR 8858 and the source of the activity was attributed to two solar flares of X-ray class M1.3 and C7.3 respectively. The CME detected on February 9 was originated in AR 8853 and flaring activity was also identified as the solar source for this event. In this study we discuss the solar origins of the events that gave rise to coronal and interplanetary disturbances and as a consequence produced geomagnetic activity at the Earth. This work is part of a complete study that is searching the solar origin, the interplanetary aspects and the magnetospheric effects of these events.
ÁreaCEA
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
IdiomaEnglish
Arquivo Alvosolar origins.pdf
Grupo de Usuáriosadministrator
alexandra
Visibilidadeshown
Detentor da CópiaSID/SCD
Política de Arquivamentodenypublisher denyfinaldraft12
Permissão de Leituradeny from all and allow from 150.163
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
DivulgaçãoWEBSCI; PORTALCAPES; SCIELO.
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 keywords label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
e-Mail (login)marciana
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