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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3QTFJHS
Repositorysid.inpe.br/mtc-m21c/2018/04.16.13.34
Metadata Repositorysid.inpe.br/mtc-m21c/2018/04.16.13.34.27
Metadata Last Update2020:12.07.21.11.28 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyMagalhãesZarEchEchGon:2018:LoFrVa
TitleLow frequency variations of Jovian radio emissions observed by Cassini
Year2018
Access Date2024, May 17
Secondary TypePRE CI
2. Context
Author1 Magalhães, Fabíola Pinho
2 Zarka, P.
3 Echer, Ezequiel
4 Echer, Mariza Pereira de Souza
5 Gonzalez Alarcon, Walter Demétrio
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
4
5 8JMKD3MGP5W/3C9JJC4
Group1 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
Affiliation1 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)
Author e-Mail Address1 fabiola.magalhaes@inpe.br
2
3 ezequiel.echer@inpe.br
4 mariza.echer@inpe.br
5 walter.gonzalez@inpe.br
Conference NameLatin American Conference on Space Geophysics, 11 (COLAGE)
Conference LocationBuenos Aires, Argentina
Date16-20 abr.
History (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
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractSince 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.
AreaCEA
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4. Conditions of access and use
Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Linking8JMKD3MGP3W34P/3MC5SSH
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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