1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m21d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34T/4B634S8 |
Repository | sid.inpe.br/mtc-m21d/2024/04.17.14.25 |
Metadata Repository | sid.inpe.br/mtc-m21d/2024/04.17.14.25.40 |
Metadata Last Update | 2024:04.19.09.15.02 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | JácomeZaLoMaEcLa:2024:DeVaEf |
Title | Declination Variation Effect on the Observation of Jovian Decametric Radio Emission |
Year | 2024 |
Access Date | 2024, May 17 |
Secondary Type | PRE CI |
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2. Context | |
Author | 1 Jácome, Hadassa Raquel Peixoto 2 Zarka, Philippe 3 Louis, Corentin K. 4 Marques, Manilo Soares 5 Echer, Ezequiel 6 Lamy, Laurent |
Resume Identifier | 1 2 3 4 5 8JMKD3MGP5W/3C9JH3D |
Group | 1 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR 2 3 4 5 DIHPA-CGCE-INPE-MCTI-GOV-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 3 4 5 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 hadassa.jacome@inpe.br 2 3 vania.andrioli@inpe.br 4 5 ezequiel.echer@inpe.br |
Conference Name | Conferencia Latinoamericana de Geofísica Espacial, 14 |
Conference Location | Monterrey, Mexico |
Date | 08-12 Apr. 2024 |
Book Title | Proceedings |
History (UTC) | 2024-04-17 14:25:40 :: simone -> administrator :: 2024-04-19 09:15:02 :: administrator -> simone :: 2024 |
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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 |
Version Type | publisher |
Abstract | The 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Declination Variation Effect... |
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 |
Visibility | shown |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | urlib.net/www/2021/06.04.03.40.25 |
Next Higher Units | 8JMKD3MGPCW/3F2PBEE |
Host Collection | urlib.net/www/2021/06.04.03.40 |
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6. Notes | |
Empty Fields | archivingpolicy 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 |
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7. Description control | |
e-Mail (login) | simone |
update | |
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