| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | mtc-m21b.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 8JMKD3MGP5W34M/3HE6FL7 |
| Repositório | sid.inpe.br/mtc-m21b/2014/11.19.00.01.26 (acesso restrito) |
| Última Atualização | 2015:02.11.11.47.14 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m21b/2014/11.19.00.01.27 |
| Última Atualização dos Metadados | 2018:06.04.03.04.34 (UTC) administrator |
| DOI | 10.1016/j.pss.2014.05.015 |
| ISSN | 0032-0633 |
| Rótulo | scopus 2014-11 HessEchZarLamDel:2014:MuStJo |
| Chave de Citação | HessEchZarLamDel:2014:MuStJo |
| Título | Multi-instrument study of the Jovian radio emissions triggered by solar wind shocks and inferred magnetospheric subcorotation rates  |
| Ano | 2014 |
| Data de Acesso | 11 maio 2024 |
| Tipo de Trabalho | journal article |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 5077 KiB |
| 2. Contextualização | |
| Autor | 1 Hess, S. L. G. 2 Echer, Ezequiel 3 Zarka, P. 4 Lamy, L. 5 Delamere, P. A. |
| Identificador de Curriculo | 1 2 8JMKD3MGP5W/3C9JH3D |
| Grupo | 1 2 DGE-CEA-INPE-MCTI-GOV-BR |
| Afiliação | 1 LESIA, Observatoire de Paris, Université Paris Diderot 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 LESIA, Observatoire de Paris, Université Paris Diderot 4 LESIA, Observatoire de Paris, Université Paris Diderot 5 University of Alaska |
| Endereço de e-Mail do Autor | 1 sebastien.hess@obspm.fr 2 eecher@dge.inpe.br |
| Endereço de e-Mail | marcelo.pazos@inpe.br |
| Revista | Planetary and Space Science |
| Volume | 99 |
| Páginas | 136-148 |
| Nota Secundária | A2_GEOCIÊNCIAS A2_INTERDISCIPLINAR B1_BIODIVERSIDADE B1_MATEMÁTICA_/_PROBABILIDADE_E B1_BIOTECNOLOGIA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ASTRONOMIA_/_FÍSICA B2_ENSINO B2_CIÊNCIAS_BIOLÓGICAS_II |
| Histórico (UTC) | 2018-06-04 03:04:34 :: administrator -> marcelo.pazos@inpe.br :: 2014 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Tipo do Conteúdo | External Contribution |
| Tipo de Versão | publisher |
| Palavras-Chave | Magnetosphere Radio astronomy Solar wind Spacecraft Storms Jovian radio arcs Jupiter-Io interaction Magnetospheric dynamics Shocks Subcorotation Interplanetary flight |
| Resumo | The influence of solar wind conditions on the Jovian auroral radio emissions has long been debated, mostly because it has always been difficult to get accurate solar wind and radio observations at the same time. We present here a study of Jupiter's radio emissions compared to solar wind conditions using radio (RPWS) and magnetic (MAG) data from the Cassini spacecraft from October to December 2000, just before its flyby of Jupiter. The spacecraft was then in the solar wind and could record both the radio emissions coming from the Jovian magnetosphere and the solar wind magnetic field (IMF). With these data, we found a good correspondence between the arrival of interplanetary shocks at Jupiter and the occurrence of radio storms. Our results confirm those from the previous studies showing that fast forward shocks (FFS) trigger mostly dusk emissions, whereas fast reverse shocks (FRS) trigger both dawn and dusk emissions. FFS-triggered emissions are found to occur 10-30 h after the shock arrival when the IMF is weak (below 2 nT), and quasi-immediately after shock arrival when the IMF is strong (above 2 nT). FRS-triggered emissions are found to occur quasi-immediately even when the IMF is weak. We show and discuss in depth the characteristic morphologies of the radio emissions related to each type of shock and their implications. We also used simultaneous radio observations from the ground-based Nançay decameter array and from the Galileo radio instrument (PWS). From the comparison of these measurements with Cassini's, we deduce the regions where the radio storms occur, as well as the radio source subcorotation rates. We show that FFS-triggered emissions onset happens in a sector of local time centered around 15:00 LT, and that all the shock-triggered radio sources sub-corotate with a subcorotation rate of ~50% when the IMF is below 2 nT and of ~80% when it is above 2 nT. These rates could correspond to the extended and compressed states of the Jovian magnetosphere. © 2014 Elsevier Ltd. All rights reserved. |
| Área | CEA |
| Arranjo | urlib.net > DIDGE > Multi-instrument study of... |
| Conteúdo da Pasta doc | acessar |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| Idioma | en |
| Arquivo Alvo | Hess_Multiinstrument.pdf |
| Grupo de Usuários | administrator marcelo.pazos@inpe.br |
| Grupo de Leitores | administrator marcelo.pazos@inpe.br |
| Visibilidade | shown |
| Política de Arquivamento | denypublisher denyfinaldraft24 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Vinculação | Trabalho não Vinculado à Tese/Dissertação |
| Repositório Espelho | iconet.com.br/banon/2006/11.26.21.31 |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
| Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 5 sid.inpe.br/bibdigital/2013/10.01.22.11 2 |
| Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. |
| Acervo Hospedeiro | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarytype url |
| 7. Controle da descrição | |
| e-Mail (login) | marcelo.pazos@inpe.br |
| atualizar | |