1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m16.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Repository | sid.inpe.br/mtc-m16@80/2006/08.11.13.37 |
Last Update | 2006:08.11.13.37.05 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m16@80/2006/08.11.13.37.06 |
Metadata Last Update | 2018:06.05.01.17.01 (UTC) administrator |
Secondary Key | INPE-14054--PRE/9224 |
Citation Key | KorthFrEcGuFrRe:2006:ClObPl |
Title | Cluster observations of plasma sheet activity during the September 14-28, 2003, corotating high speed streams event |
Year | 2006 |
Access Date | 2024, May 17 |
Secondary Type | PRE CI |
Number of Files | 1 |
Size | 1100 KiB |
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2. Context | |
Author | 1 Korth, Axel 2 Franz, M. 3 Echer, Ezequiel 4 Guarnieri, Fernando Luís 5 Friedel, R. 6 Reme, H. |
Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JH3D |
Group | 1 2 3 DGE-INPE-MCT-BR 4 DGE-INPE-MCT-BR |
Affiliation | 1 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 Name | International Conference on Substorms, 8. |
Date | 2006-03-27 |
Book Title | Proceedings |
Tertiary Type | Oral Session |
History (UTC) | 2006-08-11 13:37:06 :: simone -> administrator :: 2018-06-05 01:17:01 :: administrator -> marciana :: 2006 |
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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 |
Keywords | substorms plasma sheet geosynchronous orbit |
Abstract | Corotating 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Cluster observations of... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
data URL | http://urlib.net/ibi/sid.inpe.br/mtc-m16@80/2006/08.11.13.37 |
zipped data URL | http://urlib.net/zip/sid.inpe.br/mtc-m16@80/2006/08.11.13.37 |
Language | en |
Target File | Cluster observations of plasma sheet.pdf |
User Group | administrator simone |
Visibility | shown |
Copy Holder | SID/SCD |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3EU29DP |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 2 |
Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
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6. Notes | |
Empty Fields | archivingpolicy 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 |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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