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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3P6MU4H
Repositorysid.inpe.br/mtc-m21b/2017/06.26.18.25
Metadata Repositorysid.inpe.br/mtc-m21b/2017/06.26.18.25.53
Metadata Last Update2018:06.04.02.27.31 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyZarkaMLRLECHCD:2017:RaEmGa
TitleRadio emission from the Ganymede-Jupiter interaction and consequence for radio emissions from exoplanets
Year2017
Access Date2024, May 17
Secondary TypePRE CI
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 NameMagnetospheres of the Outer Planets (MOP)
Conference LocationUppsala, Sweden
Date12-16 june
History (UTC)2017-06-26 18:26:19 :: simone -> administrator :: 2017
2018-06-04 02:27:31 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractAnalysis 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.
AreaCEA
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4. Conditions of access and use
Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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