1. Identificação | |
Tipo de Referência | Artigo em Evento (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/3QTFJHS |
Repositório | sid.inpe.br/mtc-m21c/2018/04.16.13.34 |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2018/04.16.13.34.27 |
Última Atualização dos Metadados | 2020:12.07.21.11.28 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
Chave de Citação | MagalhãesZarEchEchGon:2018:LoFrVa |
Título | Low frequency variations of Jovian radio emissions observed by Cassini |
Ano | 2018 |
Data de Acesso | 18 maio 2024 |
Tipo Secundário | PRE CI |
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2. Contextualização | |
Autor | 1 Magalhães, Fabíola Pinho 2 Zarka, P. 3 Echer, Ezequiel 4 Echer, Mariza Pereira de Souza 5 Gonzalez Alarcon, Walter Demétrio |
Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JH3D 4 5 8JMKD3MGP5W/3C9JJC4 |
Grupo | 1 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 2 3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 5 DIDGE-CGCEA-INPE-MCTIC-GOV-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 Instituto Nacional de Pesquisas Espaciais (INPE) |
Endereço de e-Mail do Autor | 1 fabiola.magalhaes@inpe.br 2 3 ezequiel.echer@inpe.br 4 mariza.echer@inpe.br 5 walter.gonzalez@inpe.br |
Nome do Evento | Latin American Conference on Space Geophysics, 11 (COLAGE) |
Localização do Evento | Buenos Aires, Argentina |
Data | 16-20 abr. |
Histórico (UTC) | 2018-04-16 13:34:43 :: simone -> administrator :: 2018 2018-04-18 05:03:01 :: administrator -> administrator] :: 2018 2018-04-18 05:03:01 :: administrator] -> administrator :: 2018 2018-07-04 17:51:12 :: administrator -> simone :: 2018 2019-01-07 12:14:35 :: simone -> administrator :: 2018 2020-12-07 21:11:28 :: administrator -> simone :: 2018 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Resumo | Since the 1950s, Jupiter is known to be a major source of radio emissions. First, ground-based antennas obtained radio observations. Later the knowledge about plasma sources on Jupiters magnetosphere were based on in-situ and remote sensing measurements onboard spacecrafts. The radio spectrum of Jupiter spanning the frequency range from 10 kHz to 3 GHz is dominated by strong non-thermal radiation. Jupiters giant magnetosphere is mostly determined by internal interactions, primarily due to activity in Ios volcanoes, affecting the supply of plasma to all other regions. However, the Jovian magnetosphere dynamics is believed to be in part responsive changes in Solar Wind conditions. In the end of the year 2000, Cassini-Huygens spacecraft performed its closest approach to Jupiter, reaching a distance of ten million kilometers of the planet. During Cassinis flyby at the Jovian system, the Radio and Plasma Wave Science (the acronym RPWS) instrument measured Jovians radio emissions during the inbound and outbound trajectories. The present work aims to investigate Jupiters radio emissions long term variation (¿ 1 Jupiter rotation), analyzing the behaviour of the 10- hour integrated fluxes to the DAM, HOM, nKOM and bKOM bands. The data period used goes from October 2000 to March 2001. Averaged fluxes are compared for inbound and outbound orbits Correlation and Lomb-Scargle periodogram analyses were applied to RPWS data to investigate the correlation among different spectral ranges and the major periodicities. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Low frequency variations... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Low frequency variations... |
Conteúdo da Pasta doc | não têm arquivos |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Vinculação | 8JMKD3MGP3W34P/3MC5SSH |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3F2PBEE |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarytype type url versiontype volume |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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