1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34R/3SETPLP |
Repository | sid.inpe.br/mtc-m21c/2018/12.27.12.44 |
Metadata Repository | sid.inpe.br/mtc-m21c/2018/12.27.12.44.29 |
Metadata Last Update | 2021:02.27.05.02.19 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | RodríguezGómesEcheMagaMarq:2018:StSoWi |
Title | A study of solar wind effects of Jupiter magnetosphere |
Year | 2018 |
Access Date | 2024, May 16 |
Secondary Type | PRE CN |
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2. Context | |
Author | 1 Rodríguez Gómes, Jenny Marcela 2 Echer, Ezequiel 3 Magalhães, Fabíola Pinho 4 Marques, M. |
Resume Identifier | 1 2 8JMKD3MGP5W/3C9JH3D |
Group | 1 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 3 GES-CEA-SESPG-INPE-MCTIC-GOV-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Universidade Federal do Rio Grande do Norte (UFRN) |
Author e-Mail Address | 1 jemfisi@gmail.com 2 ezequiel.echer@inpe.br 3 alisson.dallago@inpe.br |
Conference Name | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 7 (SBGEA) |
Conference Location | Santa Maria, RS |
Date | 05-09 nov |
History (UTC) | 2018-12-27 12:44:29 :: simone -> administrator :: 2021-02-27 05:02:19 :: administrator -> simone :: 2018 |
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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 Sun drives many phenomena in the solar system. Its influence is mainly due to the magnetic phenomena. The solar wind interaction with the bodies of the solar system results in the formation of the magnetospheres. The Jupiter's magnetosphere in part is sensitive to the solar wind dynamic pressure variations. Several observations shown that aurora and radio emissions are intensified during higher solar wind pressure or induced by interplanetary shocks. Interplanetary shocks are driven by ICMEs or CIRS. The fast forward (FS) shock is mainly by ICMEs originated from CMEs. However, when CHs are evolving, fast streams emanate, and intercept the ambient solar wind. This interaction forms a compression region between the high speed stream and slow speed stream, it is limited by fast forward (FS) and fast reverse (RS) shocks. We present a study of fast forward and reverse shocks on the Jupiter magnetosphere. For this purpose, we use the propagated solar wind from Michigan Solar Wind model (mSWim) during the outbound period of the Cassini spacecraft. Also, the dynamic pressure will be obtained and analyzed. This work can contribute to understanding the complex Jupiter magnetosphere and its interaction with the solar wind. |
Area | CEA |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > A study of... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > A study of... |
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 | pt |
User Group | simone |
Visibility | shown |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3F2PBEE |
Citing Item List | |
Host Collection | urlib.net/www/2017/11.22.19.04 |
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6. Notes | |
Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository 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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