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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3PFBEPB
Repositóriosid.inpe.br/mtc-m21b/2017/08.18.17.39
Última Atualização2017:08.18.17.39.54 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21b/2017/08.18.17.39.54
Última Atualização dos Metadados2021:07.28.23.02.13 (UTC) administrator
DOI10.1051/0004-6361/201630025
ISSN0004-6361
1432-0746
Chave de CitaçãoMarquesZaEcRyAlDeCo:2017:StAn26
TítuloStatistical analysis of 26 yr of observations of decametric radio emissions from Jupiter
Ano2017
MêsAug.
Data de Acesso29 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho28778 KiB
2. Contextualização
Autor1 Marques, Manilo Soares
2 Zarka, Philippe
3 Echer, Ezequiel
4 Ryabov, V. B.
5 Alves, Maria Virgínia
6 Denis, L.
7 Coffre, A.
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JH3D
4
5 8JMKD3MGP5W/3C9JHRS
Grupo1 GES-CEA-SESPG-INPE-MCTIC-GOV-BR
2
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
4
5 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 LESIA, Observatoire de Paris
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Future Univ. Hakodate
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Station de Radioastronomie de Nançay, Obs. Paris, CNRS
7 Station de Radioastronomie de Nançay, Obs. Paris, CNRS
Endereço de e-Mail do Autor1 manilo.marques@gmail.com
2 philippe.zarka@obspm.fr
3 ezequiel.echer@inpe.br
4
5 mvirginia.alves@inpe.br
RevistaAstronomy & Astrophysics
Volume604
PáginasArticle number A17
Nota SecundáriaA1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_INTERDISCIPLINAR A2_ENGENHARIAS_IV A2_ASTRONOMIA_/_FÍSICA B2_ENSINO C_ENGENHARIAS_II
Histórico (UTC)2017-08-18 17:39:54 :: simone -> administrator ::
2017-08-18 17:39:55 :: administrator -> simone :: 2017
2017-08-18 17:40:58 :: simone -> administrator :: 2017
2021-07-28 23:02:13 :: administrator -> simone :: 2017
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-Chaveradiation mechanisms: non-thermal
methods: statistical
catalogs
planets and satellites: aurorae
planets and satellites: individuals: Jupiter
ResumoJupiter is a complex and at the same time very powerful radio source in the decameter wavelength range. The emission is anisotropic, intrinsically variable at millisecond to hour timescales, and also modulated by various external processes at much longer periods, ranging from ∼10 h to months or years (including Jovian day and year, solar activity and solar wind variations, and for groundbased observations, terrestrial day and year). As a consequence, long-term observations and their statistical study have proved to be necessary for disentangling and understanding the observed phenomena. We have built a database from the available 26 yr of systematic, daily observations conducted at the Nançay Decameter Array and recorded in digital format. This database contains all observed Jovian decametric emissions, classified with respect to the time-frequency morphology, their dominant circular polarization, and maximum frequency. We present the results of the first statistical analysis of this database. We confirm the earlier classification of Jovian decameter emissions in Io-A, -A0 , -B, -C, -D and non-Io-A, -B, -C types, but we also introduce new emission types (Io-A00 and Io-B0 ) and precise and characterize the non-Io-D type. We determine the contours of all emission types in the CML−ΦIo plane (Central Meridian Longitude in Jupiters System III coordinates versus Io Phase), provide representative examples of their typical time-frequency patterns, and the distribution of emissions maximum frequency as a function of ΛIo (Ios Longitude). Finally, we present a statistical analysis of the distributions of the occurrence rate, duration, intensity and polarization for each emission type. non-Io-DAM appears to be related to small-scale, possibly bursty auroral structures.
ÁreaCEA
Arranjo 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Statistical analysis of...
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 18/08/2017 14:39 1.0 KiB 
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34P/3PFBEPB
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34P/3PFBEPB
Idiomaen
Arquivo Alvomarques_statistical.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.55.54 4
sid.inpe.br/bibdigital/2013/10.01.22.11 3
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 3
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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