| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34T/45NLA98 | |||
| Repository | sid.inpe.br/mtc-m21d/2021/11.05.11.34 | |||
| Last Update | 2021:11.05.11.34.26 (UTC) administrator | |||
| Metadata Repository | sid.inpe.br/mtc-m21d/2021/11.05.11.34.26 | |||
| Metadata Last Update | 2022:04.15.08.28.04 (UTC) administrator | |||
| DOI | 10.1029/2021JA029780 | |||
| ISSN | 2169-9402 | |||
| Citation Key | ZarkaMMLELCP:2021:RoVeSo | |||
| Title | Jupiter's Auroral Radio Emissions Observed by Cassini: Rotational Versus Solar Wind Control, and Components Identification  | |||
| Year | 2021 | |||
| Month | Oct. | |||
| Access Date | 2024, May 17 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 8455 KiB | |||
| 2. Context | ||||
| Author | 1 Zarka, P. 2 Magalhães, F. P. 3 Marques, M. S. 4 Louis, C. K. 5 Echer, Ezequiel 6 Lamy, L. 7 Cecconi, B. 8 Prangé, R. | |||
| Resume Identifier | 1 2 3 4 5 8JMKD3MGP5W/3C9JH3D | |||
| ORCID | 1 0000-0003-1672-9878 2 0000-0002-6328-0041 3 0000-0003-4896-7301 4 0000-0002-9552-8822 5 0000-0002-8351-6779 6 0000-0002-8428-1369 7 0000-0001-7915-5571 8 0000-0001-8809-4563 | |||
| Group | 1 2 3 4 5 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 Sorbonne Université 2 Sorbonne Université 3 Universidade Federal do Rio Grande do Norte (UFRN) 4 Université de Toulouse 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Sorbonne Université 7 Sorbonne Université 8 Sorbonne Université | |||
| Author e-Mail Address | 1 philippe.zarka@obspm.fr 2 3 4 5 ezequiel.echer@inpe.br | |||
| Journal | Journal of Geophysical Research: Space Physics | |||
| Volume | 126 | |||
| Number | 10 | |||
| Pages | e2021JA029780 | |||
| History (UTC) | 2021-11-05 11:34:26 :: simone -> administrator :: 2021-11-05 11:34:28 :: administrator -> simone :: 2021 2021-11-05 11:35:21 :: simone -> administrator :: 2021 2022-04-15 08:28:04 :: administrator -> simone :: 2021 | |||
| 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 | |||
| Keywords | 2736 2756 2784 7534 auroral radio emissions Jupiter radio components magnetospheric dynamics rotation control solar wind control | |||
| Abstract | Reanalyzing Cassini radio observations performed during Jupiter's flyby of 20002001, we study the internal (rotational) versus external (solar wind) control of Jupiter's radio emissions, from kilometer to decameter wavelengths, and the relations between the different auroral radio components. For that purpose, we build a database of the occurrence of Jovian auroral radio components bKOM, HOM, and DAM observed by Cassini, and then frequency-longitude stacked plots of the polarized intensity of these radio components. Comparing the results obtained inbound and outbound, as a function of the Observer's or Sun's longitude, we find that HOM & DAM are dominantly rotation-modulated (i.e., emitted from searchlight-like sources fixed in Jovian longitude), whereas bKOM is modulated more strongly by the solar wind than by the rotation (i.e., emitted from sources more active within a given Local Time sector). We propose a simple analytical description of these internal and external modulations and evaluate its main parameters (the amplitude of each control) for HOM + DAM and bKOM. Comparing Cassini and Nançay Decameter Array data, we find that HOM is primarily connected to the decameter emissions originating from the dusk sector of the Jovian magnetosphere. HOM and DAM components form a complex but stable pattern in the frequency-longitude plane. HOM also seems to be related to the lesser arcs identified by Voyager. bKOM consists of a main part above (Formula presented.) 40 kHz in antiphase with HOM occurrence, and detached patches below (Formula presented.) 80 kHz in phase with HOM. The frequency-longitude patterns formed by DAM, HOM and bKOM remain to be modeled. | |||
| Area | CEA | |||
| Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Jupiter's Auroral Radio... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| data URL | http://urlib.net/ibi/8JMKD3MGP3W34T/45NLA98 | |||
| zipped data URL | http://urlib.net/zip/8JMKD3MGP3W34T/45NLA98 | |||
| Language | en | |||
| Target File | zarka_jupiter.pdf | |||
| User Group | simone | |||
| Visibility | shown | |||
| Archiving Policy | denypublisher6 allowfinaldraft | |||
| Read Permission | allow from all | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/46KTFK8 | |||
| Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 7 | |||
| Dissemination | WEBSCI; AGU; MGA; COMPENDEX. | |||
| Host Collection | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||