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1. Identity statement
Reference TypeSlides (Audiovisual Material)
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP8W/34B6KD8
Repositorysid.inpe.br/mtc-m18@80/2008/12.02.15.25   (restricted access)
Last Update2008:12.02.15.25.56 (UTC) seeger05
Metadata Repositorysid.inpe.br/mtc-m18@80/2008/12.02.15.25.58
Metadata Last Update2018:06.04.04.05.47 (UTC) administrator
Secondary KeyINPE--MAO/
Citation KeyKummerSELBSKSBS:2008:StJuMa
TitleA study of Jupiter’s magnetopause orientation and position
FormatOn-line
Year2008
Access Date2024, Apr. 27
Number of Files1
Size622 KiB
2. Context
Author 1 Kummer, Fabrício Deives
 2 Schuch, Nelson Jorge
 3 Echer, Ezequiel
 4 Lago, Alisson Dal
 5 Battistel, Orimar Antonio
 6 Silva, Samuel Martins da
 7 Kemmerich, Níkolas
 8 Silveira, Marcos Vinicius dias
 9 Braga, Carlos Roberto
10 Silva, Marlos Rockenbach da
Group 1 RSU-CIE-INPE-MCT-BR
 2 RSU-CIE-INPE-MCT-BR
 3 DGE-CEA-INPE-MCT-BR
 4 DGE-CEA-INPE-MCT-BR
 5
 6 RSU-CIE-INPE-MCT-BR
 7 RSU-CIE-INPE-MCT-BR
 8 RSU-CIE-INPE-MCT-BR
 9 RSU-CIE-INPE-MCT-BR
10 DGE-CEA-INPE-MCT-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2
 3
 4
 5 Universidade Fedral de Santa Maria
Conference NameScientific Assembly of COSPAR, (37Th).
Conference LocationMontreal, Canada
Date18-25, July
PublisherInstituto Nacional de Pesquisas Espaciais
Publisher CitySão José dos Campos
History (UTC)2008-12-03 19:55:56 :: seeger05 -> administrator ::
2018-06-04 04:05:47 :: administrator -> seeger05 ::
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
AbstractThe solar wind is a supersonic magnetized fluid which continuously flow outwards from the solar atmosphere. When the solar wind flows through the solar system and encounters an obstacle such as a planetary magnetic field, a magnetosphere is formed. The boundary between the solar wind and a planetary plasma environments is the magnetopause. At this boundary, mass, momentum and energy exchange between the solar wind and the planetary environment occur. Jupiter has the largest and more complex magnetosphere of the solar system. The position and shape of Jupiters magnetopause is determined by a balance between the solar wind dynamic pressure and the internal, magnetic plus plasma pressure of Jupiter magnetopshere. The objective of this work is to study the orientation and position of the Jupiter magnetopause, using magnetic field observations and the minimum variance analysis. To conduct this study,we use magnetopause crossing data from the Voyager-1, Voyager-2 and Ulysses spacecraft. Finally, the position of the magnetopause is investigated in relation to the ambient solar wind conditions.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > A study of...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > A study of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FilePôster COSPAR 2008_Fabricio Deives Kummer - 505.ppt
User Groupseeger05
Visibilityshown
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
NotesISSN 1815-2619
Empty Fieldsarchivingpolicy archivist booktitle callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress electronicmailaddress isbn issn keywords label lineage mark mirrorrepository nextedition numberofslides orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark secondarytype session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
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