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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/38Q5L7P
Repositóriosid.inpe.br/mtc-m19/2010/12.16.15.26
Última Atualização2011:03.01.20.09.31 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2010/12.16.15.26.13
Última Atualização dos Metadados2018:06.05.04.34.57 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1051/0004-6361/200913305
ISSN0004-6361
1432-0746
Chave de CitaçãoEcher:2010:SoWiEf
TítuloSolar wind effects on Jupiter non-Io DAM emissions during Ulysses distant encounter (2003-2004)
Ano2010
MêsSet.
Data de Acesso20 maio 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho604 KiB
2. Contextualização
AutorEcher, Ezequiel
Identificador de Curriculo8JMKD3MGP5W/3C9JH3D
GrupoDGE-CEA-INPE-MCT-BR
AfiliaçãoInstituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Maillise@dpi.inpe.br
RevistaAstronomy & Astrophysics
Volume519
NúmeroA84
Páginas8
Histórico (UTC)2011-01-05 12:30:13 :: marciana -> administrator :: 2010
2011-02-26 22:28:34 :: administrator -> marciana :: 2010
2011-03-01 20:06:09 :: marciana -> lise@dpi.inpe.br :: 2010
2011-09-13 12:40:31 :: lise@dpi.inpe.br -> marciana :: 2010
2012-01-26 10:55:24 :: marciana -> administrator :: 2010
2018-06-05 04:34:57 :: administrator -> marciana :: 2010
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chaveplanets and satellites: general
solar wind
DECAMETRIC RADIO-EMISSION
BROAD-BAND
MAGNETOSPHERE
ORIGIN
SHOCKS
STORMS
ResumoAims. We analyze solar wind data from the Ulysses spacecraft during the distant Jupiter encounter from 2003 November to 2004 March as well as Nancay decametric (DAM) radio observations non-controlled by Io. Methods. The Ulysses solar wind data are balistically propagated towards Jupiter and are correlated with Nancay non-Io DAM emissions. Results. It is found that the average solar wind dynamic pressure around the time of DAM emissions is 1.7 times higher than its average value during the Ulysses encounter. The occurrence of fast forward (FS) and reverse (RS) interplanetary shocks and heliospheric current sheet crossings (HCS) is correlated with the occurrence of non-Io DAM emissions. We note an enhanced probability of occurrence of non-Io DAM emissions after the expected arrival of FS, RS and HCS at Jupiter. However, about half emissions (54%) did not seem to be associated with these interplanetary structures. We also note that the average duration and power of non-Io DAM emissions are enhanced during periods associated with those interplanetary structures. Conclusions. From the results obtained in this work it seems that non-Io DAM emissions occur during intervals of enhanced solar wind dynamic pressure. Yet, there is no direct correlation between the non-Io DAM emissions duration or power versus the solar wind pressure values and the interplanetary shock Mach number.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Solar wind effects...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 16/12/2010 13:26 1.0 KiB 
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP7W/38Q5L7P
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP7W/38Q5L7P
Idiomaen
Arquivo Alvo12.16.15.26__0004-6361.pdf
Grupo de Usuáriosadministrator
lise@dpi.inpe.br
marciana
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhosid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 2
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
DivulgaçãoWEBSCI; PORTALCAPES.
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
e-Mail (login)marciana
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