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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/mtc-m16@80/2006/08.11.13.37
Last Update2006:08.11.13.37.05 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/08.11.13.37.06
Metadata Last Update2018:06.05.01.17.01 (UTC) administrator
Secondary KeyINPE-14054--PRE/9224
Citation KeyKorthFrEcGuFrRe:2006:ClObPl
TitleCluster observations of plasma sheet activity during the September 14-28, 2003, corotating high speed streams event
Year2006
Access Date2024, May 17
Secondary TypePRE CI
Number of Files1
Size1100 KiB
2. Context
Author1 Korth, Axel
2 Franz, M.
3 Echer, Ezequiel
4 Guarnieri, Fernando Luís
5 Friedel, R.
6 Reme, H.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
Group1
2
3 DGE-INPE-MCT-BR
4 DGE-INPE-MCT-BR
Affiliation1 Max-Planck-Institut für Sonnesystemforschung
2
3 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
4 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
Conference NameInternational Conference on Substorms, 8.
Date2006-03-27
Book TitleProceedings
Tertiary TypeOral Session
History (UTC)2006-08-11 13:37:06 :: simone -> administrator ::
2018-06-05 01:17:01 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordssubstorms
plasma sheet
geosynchronous orbit
AbstractCorotating Interaction Regions (CIR's) are large scale structures in the heliosphere during the declining and minimum phase of the solar activity cycle. They are the result of the interaction of fast and slow solar wind. Streams of fast solar wind originating from coronal holes often recurred with a period of ~ 27 days, the solar rotation. These streams of fast solar wind and the interplanetary field will influence the dynamics of the Earth's magnetosphere. We will present magnetospheric conditions during high speed streams in September 2003 and will show Cluster ion data in the energy range from 30 eV to 500 keV and electrons from 30 keV to 300 keV in the plasma sheet of the magnetosphere at ~ 20 RE. The pressure change in the plasma sheet is correlated with injections at geosynchronous orbit. A cross-wavelet analysis between the interplanetary magnetic field IMF Bz and the sunward component Bx from Cluster in the plasma heet show a high correlation at about two hours.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Cluster observations of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/mtc-m16@80/2006/08.11.13.37
zipped data URLhttp://urlib.net/zip/sid.inpe.br/mtc-m16@80/2006/08.11.13.37
Languageen
Target FileCluster observations of plasma sheet.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber conferencelocation copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url versiontype volume
7. Description control
e-Mail (login)marciana
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