| 1. Identificação | ||||
| Tipo de Referência | Artigo em Evento (Conference Proceedings) | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identificador | 8JMKD3MGP3W34T/453QSJ8 | |||
| Repositório | sid.inpe.br/mtc-m21d/2021/07.12.15.55 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21d/2021/07.12.15.55.31 | |||
| Última Atualização dos Metadados | 2022:04.03.19.24.48 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | JàcomeMarEchLamZar:2021:CoJoRa | |||
| Título | Compilation of Jovian radio Decametric emissions with complete arcs in dynamic spectra observed by Wind/WAVES/RAD2 and the Nançay Decameter Array – A3  | |||
| Ano | 2021 | |||
| Data de Acesso | 18 maio 2024 | |||
| Tipo Secundário | PRE CI | |||
| 2. Contextualização | ||||
| Autor | 1 Jàcome, H. R. P. 2 Marques, M. S. 3 Echer, Ezequiel 4 Lamy, L. 5 Zarka, P. | |||
| Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JH3D | |||
| Grupo | 1 2 3 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 Universidade Federal do Rio Grande do Norte (UFRN) 2 Universidade Federal do Rio Grande do Norte (UFRN) 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 LESIA, Observatoire de Paris 5 LESIA, Observatoire de Paris | |||
| Endereço de e-Mail do Autor | 1 2 3 ezequiel.echer@gmail.com | |||
| Nome do Evento | Magnetospheres of Outer Planets Meeting | |||
| Localização do Evento | Online | |||
| Data | 12-16 July | |||
| Título do Livro | Proceedings | |||
| Histórico (UTC) | 2021-07-12 15:56:04 :: simone -> administrator :: 2021 2022-04-03 19:24:48 :: administrator -> simone :: 2021 | |||
| 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 | The plasma-satellite electrodynamic interactions that occur inside the Jovian magnetosphere with the Galilean satellites produce field-aligned electric currents that are carried by Alfvén waves towards Jupiters ionosphere, accelerating electrons and causing auroral emissions at UV, IR and radio wavelengths. The Jovian Decametric (DAM) radio emissions are produced by electron-wave resonance through the Cyclotron Maser Instability (CMI) at the local electron cyclotron frequency. These emissions have frequencies from a few MHz to ∼40 MHz, and, therefore, are partially observed from the Earth >10 MHz. The long-term monitoring of Jupiter by the Nançay Decametric Array has enabled to collect more than 40 years of daily observations of Jupiter between 10 and 40 MHz. The last 30 years of observations (since 1990) compose the NDAs extensive digital catalog, which based the in depth study of the various Jovian DAM components, and provided evidences of emissions driven by Io, Europa and Ganymede. However, radio observations from ground-based instruments such as the NDA are limited by the terrestrial ionospheres cutoff frequency, of ∼10 MHz, and by Radio Frequency Interference (RFI) up to ∼20 MHz. In this context, the complementary use of observations from spacecraft-based radio instruments emerges as an interesting possibility to improve the analysis of planetary radio emissions by overcoming the frequency limitation of terrestrial observations. Wind is a spacecraft that has been on space, at the vicinity of the Earth, since the end of 1994, collecting radio DAM emissions with frequencies up to 14 MHz through the onboard WAVES experiment, whose frequency range coverage comprises part of the Jovian DAM emission that is not detectable by the NDA. Jupiter is observed by Wind in some parts of the spacecrafts orbit, making it possible for WAVES receivers to occasionally detect Jovian DAM emissions at low frequencies. Therefore, this work aims at producing a catalog of Jovian DAM emissions observed by both the NDA and Wind to improve the analysis of the emissions controlled by the Galilean satellites that have been observed on the NDAs catalog, by extending these emissions to their lower frequencies observed by Wind. This extension enables the visualization of the entire frequency range of the emissions and a more complete analysis of their arc shapes formed in the dynamic spectra. | |||
| Área | CEA | |||
| Arranjo | urlib.net > CGCE > Compilation of Jovian... | |||
| 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 | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/46KTFK8 | |||
| Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notas | ||||
| Campos Vazios | archivingpolicy archivist 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 tertiarymark tertiarytype type url versiontype volume | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||