| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m21b.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 8JMKD3MGP5W34M/3HE6FL7 |
| Repository | sid.inpe.br/mtc-m21b/2014/11.19.00.01.26 (restricted access) |
| Last Update | 2015:02.11.11.47.14 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m21b/2014/11.19.00.01.27 |
| Metadata Last Update | 2018:06.04.03.04.34 (UTC) administrator |
| DOI | 10.1016/j.pss.2014.05.015 |
| ISSN | 0032-0633 |
| Label | scopus 2014-11 HessEchZarLamDel:2014:MuStJo |
| Citation Key | HessEchZarLamDel:2014:MuStJo |
| Title | Multi-instrument study of the Jovian radio emissions triggered by solar wind shocks and inferred magnetospheric subcorotation rates  |
| Year | 2014 |
| Access Date | 2024, May 17 |
| Type of Work | journal article |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 5077 KiB |
| 2. Context | |
| Author | 1 Hess, S. L. G. 2 Echer, Ezequiel 3 Zarka, P. 4 Lamy, L. 5 Delamere, P. A. |
| Resume Identifier | 1 2 8JMKD3MGP5W/3C9JH3D |
| Group | 1 2 DGE-CEA-INPE-MCTI-GOV-BR |
| Affiliation | 1 LESIA, Observatoire de Paris, Université Paris Diderot 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 LESIA, Observatoire de Paris, Université Paris Diderot 4 LESIA, Observatoire de Paris, Université Paris Diderot 5 University of Alaska |
| Author e-Mail Address | 1 sebastien.hess@obspm.fr 2 eecher@dge.inpe.br |
| e-Mail Address | marcelo.pazos@inpe.br |
| Journal | Planetary and Space Science |
| Volume | 99 |
| Pages | 136-148 |
| Secondary Mark | A2_GEOCIÊNCIAS A2_INTERDISCIPLINAR B1_BIODIVERSIDADE B1_MATEMÁTICA_/_PROBABILIDADE_E B1_BIOTECNOLOGIA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ASTRONOMIA_/_FÍSICA B2_ENSINO B2_CIÊNCIAS_BIOLÓGICAS_II |
| History (UTC) | 2018-06-04 03:04:34 :: administrator -> marcelo.pazos@inpe.br :: 2014 |
| 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 | Magnetosphere Radio astronomy Solar wind Spacecraft Storms Jovian radio arcs Jupiter-Io interaction Magnetospheric dynamics Shocks Subcorotation Interplanetary flight |
| Abstract | The influence of solar wind conditions on the Jovian auroral radio emissions has long been debated, mostly because it has always been difficult to get accurate solar wind and radio observations at the same time. We present here a study of Jupiter's radio emissions compared to solar wind conditions using radio (RPWS) and magnetic (MAG) data from the Cassini spacecraft from October to December 2000, just before its flyby of Jupiter. The spacecraft was then in the solar wind and could record both the radio emissions coming from the Jovian magnetosphere and the solar wind magnetic field (IMF). With these data, we found a good correspondence between the arrival of interplanetary shocks at Jupiter and the occurrence of radio storms. Our results confirm those from the previous studies showing that fast forward shocks (FFS) trigger mostly dusk emissions, whereas fast reverse shocks (FRS) trigger both dawn and dusk emissions. FFS-triggered emissions are found to occur 10-30 h after the shock arrival when the IMF is weak (below 2 nT), and quasi-immediately after shock arrival when the IMF is strong (above 2 nT). FRS-triggered emissions are found to occur quasi-immediately even when the IMF is weak. We show and discuss in depth the characteristic morphologies of the radio emissions related to each type of shock and their implications. We also used simultaneous radio observations from the ground-based Nançay decameter array and from the Galileo radio instrument (PWS). From the comparison of these measurements with Cassini's, we deduce the regions where the radio storms occur, as well as the radio source subcorotation rates. We show that FFS-triggered emissions onset happens in a sector of local time centered around 15:00 LT, and that all the shock-triggered radio sources sub-corotate with a subcorotation rate of ~50% when the IMF is below 2 nT and of ~80% when it is above 2 nT. These rates could correspond to the extended and compressed states of the Jovian magnetosphere. © 2014 Elsevier Ltd. All rights reserved. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Multi-instrument study of... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | Hess_Multiinstrument.pdf |
| User Group | administrator marcelo.pazos@inpe.br |
| Reader Group | administrator marcelo.pazos@inpe.br |
| Visibility | shown |
| Archiving Policy | denypublisher denyfinaldraft24 |
| Read Permission | deny from all and allow from 150.163 |
| Update Permission | not transferred |
| 5. Allied materials | |
| Linking | Trabalho não Vinculado à Tese/Dissertação |
| Mirror Repository | iconet.com.br/banon/2006/11.26.21.31 |
| Next Higher Units | 8JMKD3MGPCW/3EU29DP |
| Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 5 sid.inpe.br/bibdigital/2013/10.01.22.11 2 |
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. |
| Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarytype url |
| 7. Description control | |
| e-Mail (login) | marcelo.pazos@inpe.br |
| update | |