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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/JwEKp
Repositóriosid.inpe.br/iris@1916/2005/12.21.12.35.35   (acesso restrito)
Última Atualização2005:12.22.15.35.00 (UTC) administrator
Repositório de Metadadossid.inpe.br/iris@1916/2005/12.21.12.35.41
Última Atualização dos Metadados2021:07.18.04.01.21 (UTC) administrator
Chave SecundáriaINPE-12715-PRE/8005
ISSN1364-6826
Chave de CitaçãoCecattoSoFeMaAnSa:2005:RaEmOb
TítuloRadio emission observed in decimetric waves associated with the onset of CMEs
Ano2005
Data de Acesso07 maio 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho434 KiB
2. Contextualização
Autor1 Cecatto, José Roberto
2 Soares, Alfredo de Carvalho
3 Fernandes, Francisco Carlos Rocha
4 Madsen, F. R. H.
5 Andrade, Maria Conceição de
6 Sawant, Hanumant Shankar
Identificador de Curriculo1 8JMKD3MGP5W/3C9JHJB
2
3
4
5 8JMKD3MGP5W/3C9JHR2
6 8JMKD3MGP5W/3C9JHBU
Grupo1 DAS-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE, DAS)
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Volume67
Número17-18
Páginas1673-1678
Histórico (UTC)2005-12-22 15:35:19 :: jefferson -> administrator ::
2021-07-18 04:01:21 :: 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-ChaveRadio emission
CME
Decimetric waves
Solar bursts
ResumoSince the first observations by Skylab and SMM satellites coronal mass ejections (CME) have been more and more investigated. However, until now their origin and trigger mechanism remain an open question no matter if they are associated to flares or not. Recent observations over a broad spectrum suggest that flare energy is released in regions from where the decimetric emission is coming. Then, investigations of decimetric radio emission observed in association with CME phenomena may give clues to solve the previously mentioned questions. Using the Brazilian solar spectroscope (BSS), observations of solar bursts dynamic spectra with high time (100, 50, 20 ms) and frequency (50100 channels) resolutions have been carried out daily (1119 UT) within the range of 10002500 MHz. A sample of 274 CMEs were recorded by the large angle spectroscopic coronagraph (LASCO) instrument, on board the solar and heliospheric observatory (SOHO) satellite, within 1119 UT, during the period of 19992002. From those, 42 CMEs are associated to BSS data and selected for analysis. It is interesting to note that in about half of the cases only one type of burst radio emission was recorded while in the remaining cases either two or more types were observed. There is a dominance of either continuum and/or pulsations. Here, we describe the association of burst radio emission with the starting time of CME phenomena.
ÁreaCEA
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Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Arquivo AlvoRadio emission observed.pdf
Grupo de Usuáriosadministrator
jefferson
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/3ETR8EH
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 month 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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