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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@80/2005/10.13.20.13
Last Update2006:06.14.04.43.38 (UTC) administrator
Metadata Repositorysid.inpe.br/MTC-m13@80/2005/10.13.20.13.20
Metadata Last Update2018:06.04.04.12.29 (UTC) administrator
Secondary KeyINPE-13223-PRE/8479
Citation KeyAndrioliSaviEcheSchu:2005:DeCiRe
TitleDetermination of Cir Related Shock Parameters
FormatPapel
Year2005
Access Date2024, May 17
Secondary TypePRE CI
Number of Files1
Size1019 KiB
2. Context
Author1 Andrioli, V. F.
2 Savian, Jairo Francisco
3 Echer, Ezequiel
4 Schuch, Nelson Jesus
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
Group1 DGE-INPE-MCT-BR
2 RSU-INPE-MCT-BR
Affiliation1 LACESM/CT-Universidade Federal de Santa MariaUFSM/ME,CRSPE-INPE-MCT
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial (INPE, DGE)
3 Centro Regional Sul de Pesquisas Espaciais CRSPE/INPE-MCT
Conference NameAGU Chapman Conference: Corotating Solar Wind Streams and Recurrent Geomagnetic Activity.
Conference LocationManaus
Date6 a 12 de fevereiro
Book TitleAnales
Tertiary TypeSessão Poster
History (UTC)2005-10-13 20:19:46 :: seeger05 -> marciana ::
2006-07-19 21:24:36 :: marciana -> administrator ::
2006-09-27 20:14:50 :: administrator -> marciana ::
2008-05-02 14:59:04 :: 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
AbstractDuring the descending and minimum solar cycle phase, polar coronal holes extend from the polar regions down to the solar equator. The high-speed streams emitted by coronal holes can interact with the ambient, slow solar wind streams and form corotating interaction regions (CIR). These CIRs are usually well developed only beyond 1.5 astronomical units, when a pair of reverse and fast forward shocks can form and delimit the stream interface. The stream interface is the region when the ambient solar wind is compressed by the high speed stream and as a result both magnetic field strength and density are enhanced. At the Earths orbit, 1 astronomical unit, one does not usually observe CIR related fast forward shocks, but reverse shocks are estimated to be present in 20% of the cases. In this work, we study the CIRs events of solar cycle 23 maximum and descending phases (2001-2004) to identify which is the percentage of CIRs with interplanetary shocks at Earths orbit. For the CIRs events with shocks, the interplanetary shock parameters (Mach number, magnetic field and density compression rations and shock speed) are computed. A few examples are shown that illustrate the presence of the CIR-reverse shock and also the possible presence of a pair of fast and reverse shocks.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Determination of Cir...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Determination of Cir...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/MTC-m13@80/2005/10.13.20.13
zipped data URLhttp://urlib.net/zip/sid.inpe.br/MTC-m13@80/2005/10.13.20.13
Languageen
Target Filedetermination cir.pdf
User Groupadministrator
marciana
seeger05
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
Dissemination<E>
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
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