1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m21b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34P/3P6MU4H |
Repository | sid.inpe.br/mtc-m21b/2017/06.26.18.25 |
Metadata Repository | sid.inpe.br/mtc-m21b/2017/06.26.18.25.53 |
Metadata Last Update | 2018:06.04.02.27.31 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | ZarkaMLRLECHCD:2017:RaEmGa |
Title | Radio emission from the Ganymede-Jupiter interaction and consequence for radio emissions from exoplanets |
Year | 2017 |
Access Date | 2024, May 17 |
Secondary Type | PRE CI |
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2. Context | |
Author | 1 Zarka, Philippe 2 Marques, Manilo Soares 3 Louis, Corentin 4 Ryabov, Vladimir 5 Lamy, Laurent 6 Echer, Ezequiel 7 Cecconi, Baptiste 8 Hess, Sébastien 9 Coffre, André 10 Denis, Laurent |
Resume Identifier | 1 2 3 4 5 6 8JMKD3MGP5W/3C9JH3D |
Group | 1 2 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 3 4 5 6 DIDGE-CGCEA-INPE-MCTIC-GOV-BR |
Affiliation | 1 Observatoire de Paris 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 4 5 6 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 2 3 4 5 6 ezequiel.echer@inpe.br |
Conference Name | Magnetospheres of the Outer Planets (MOP) |
Conference Location | Uppsala, Sweden |
Date | 12-16 june |
History (UTC) | 2017-06-26 18:26:19 :: simone -> administrator :: 2017 2018-06-04 02:27:31 :: administrator -> simone :: 2017 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Abstract | Analysis of a catalog of 26 years of radio decameter observations from Jupiter in Nançay (France) allowed us to detect unambiguously the radio emissions resulting from the Ganymede-Jupiter interaction. The duration and power of the 189 events detected suggest sporadic reconnection with an average radio power released in the Ganymede-Jupiter decameter emission 15 times smaller than in the Io-Jupiter one. This compares well with the ratio of the magnetic power (Poynting flux) dissipated at the Ganymede-Jupiter and Io-Jupiter interactions, confirming the radio-magnetic Bodes law of Zarka et al. (2001), that serves as a basis for predicting exoplanetary radio emissions. Constraints imposed by the Ganymede-Jupiter radio emission on Jovian magnetic field models are also discussed. |
Area | CEA |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Radio emission from... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Radio emission from... |
doc Directory Content | there are no files |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Read Permission | allow from all |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3F2PBEE |
Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notes | |
Empty Fields | 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 rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
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7. Description control | |
e-Mail (login) | simone |
update | |
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