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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/MTC-m13@80/2005/10.13.19.57
Last Update2006:06.14.04.43.30 (UTC) administrator
Metadata Repositorysid.inpe.br/MTC-m13@80/2005/10.13.19.58.01
Metadata Last Update2018:06.04.04.12.29 (UTC) administrator
Secondary KeyINPE-13176-PRE/8433
Citation KeyAndrioliSaviEzeqSchu:2005:CoStSh
TitleA Comparative Study of Shock Parameter Variations across Transient and Corotating Shocks
FormatCD-ROM, Papel.
Year2005
Access Date2024, May 18
Secondary TypePRE CI
Number of Files1
Size438 KiB
2. Context
Author1 Andrioli, V. F.
2 Savian, J.
3 Ezequiel, Echer
4 Schuch, Nelson Jorge
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHUD
Group1 DGE-INPE-MCT-BR
2 RSU-INPE-MCT-BR
Affiliation1 Universidade Federal de Santa Maria - UFSM/ME
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial (INPE, DGE)
3 Instituto Nacional de Pesquisas Espaciais, RSU
Conference NameInternational Association of Geomagnetism and Aeronomy (IAGA), 10
Conference LocationToulouse
Date18-29 july
Tertiary TypePosters
History (UTC)2005-11-17 13:34:48 :: seeger05 -> marciana ::
2005-11-18 10:01:46 :: marciana -> administrator ::
2006-09-27 20:14:48 :: administrator -> marciana ::
2008-05-02 14:59:03 :: marciana -> administrator ::
2018-06-04 04:12:29 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
AbstractIn this work we study the variations in the plasma and magnetic field parameters across transient, ICME-driven shocks (fast forward), and corotating shocks (mainly fast reverse), associated with CIRs. The period analysed is the decline phase of the solar cycle 23 (2002-2003). Solar wind data were obtained through internet from the ACE - Advanced Composition Explorer database (http://www.srl.caltech.edu/ACE/ASC/level2/index.html). We plot and analyze solar wind data and classify every shock according to its propagation direction (forward or reverse) and MHD wave mode (fast or slow). Associated solar wind structures were also determined (ICMEs or CIRs). The jump of plasma and magnetic field across hese shocks was then calculated and distributions obtained for each interplanetary shock type. These distributions are compared in this work.
AreaCEA
Arrangement 1urlib.net > DIDGE > A Comparative Study...
Arrangement 2urlib.net > Produção anterior à 2021 > CRCRS > A Comparative Study...
doc Directory Contentaccess
source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/MTC-m13@80/2005/10.13.19.57
zipped data URLhttp://urlib.net/zip/sid.inpe.br/MTC-m13@80/2005/10.13.19.57
Languageen
Target Filecomparativy study shock.pdf
User Groupadministrator
marciana
seeger05
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.02 6
sid.inpe.br/bibdigital/2013/10.04.21.53 3
Dissemination<E>
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber contenttype copyright creatorhistory descriptionlevel documentstage doi e-mailaddress edition editor electronicmailaddress identifier isbn issn keywords 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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