Close

1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4B634S8
Repositorysid.inpe.br/mtc-m21d/2024/04.17.14.25
Metadata Repositorysid.inpe.br/mtc-m21d/2024/04.17.14.25.40
Metadata Last Update2024:04.19.09.15.02 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyJácomeZaLoMaEcLa:2024:DeVaEf
TitleDeclination Variation Effect on the Observation of Jovian Decametric Radio Emission
Year2024
Access Date2024, May 17
Secondary TypePRE CI
2. Context
Author1 Jácome, Hadassa Raquel Peixoto
2 Zarka, Philippe
3 Louis, Corentin K.
4 Marques, Manilo Soares
5 Echer, Ezequiel
6 Lamy, Laurent
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JH3D
Group1 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR
2
3
4
5 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2
3
4
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 hadassa.jacome@inpe.br
2
3 vania.andrioli@inpe.br
4
5 ezequiel.echer@inpe.br
Conference NameConferencia Latinoamericana de Geofísica Espacial, 14
Conference LocationMonterrey, Mexico
Date08-12 Apr. 2024
Book TitleProceedings
History (UTC)2024-04-17 14:25:40 :: simone -> administrator ::
2024-04-19 09:15:02 :: administrator -> simone :: 2024
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe Jovian Decametric (DAM) radio emissions are anisotropically beamed emissions generated via cyclotron maser instability at Jupiters auroral regions. It is long known that the observation of these emission is affected by the variation of the observers latitude (or declination - DE) in the Jovian System III, but the declination effect is still not well understood. In this work, we analyze Jovian DAM emission detected by the Nançay Decameter Array from 1990 to 2020 and suggest a selection of the emission by intensity and maximum frequency thresholds to remove the superimposed effects of the variation of observer-Jupiter distance and of Jupiters elongation angle. Then, we study the pure effect of DE on the selected emissions duration, maximum frequency, average longitude (CML) and average Io phase. The same analysis is applied on simulations of Jovian emission by the Exoplanetary and Planetary Radio Emissions Simulator (ExPRES). ExPRES seems to predict the emission and their variation with DE consistently with what is observed in the NDA data, and might be an additional tool to confirm the theory on the emissions origin and to improve our understanding of the DE effect on the emission observation.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Declination Variation Effect...
doc Directory Contentthere are no files
source Directory Contentthere are no files
agreement Directory Content
agreement.html 17/04/2024 11:25 1.0 KiB 
4. Conditions of access and use
Languageen
User Groupsimone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2021/06.04.03.40.25
Next Higher Units8JMKD3MGPCW/3F2PBEE
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url volume
7. Description control
e-Mail (login)simone
update 


Close