1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m16c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Repository | sid.inpe.br/MTC-m13@80/2005/10.13.20.13 |
Last Update | 2006:06.14.04.43.38 (UTC) administrator |
Metadata Repository | sid.inpe.br/MTC-m13@80/2005/10.13.20.13.20 |
Metadata Last Update | 2018:06.04.04.12.29 (UTC) administrator |
Secondary Key | INPE-13223-PRE/8479 |
Citation Key | AndrioliSaviEcheSchu:2005:DeCiRe |
Title | Determination of Cir Related Shock Parameters |
Format | Papel |
Year | 2005 |
Access Date | 2024, May 17 |
Secondary Type | PRE CI |
Number of Files | 1 |
Size | 1019 KiB |
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2. Context | |
Author | 1 Andrioli, V. F. 2 Savian, Jairo Francisco 3 Echer, Ezequiel 4 Schuch, Nelson Jesus |
Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JH3D |
Group | 1 DGE-INPE-MCT-BR 2 RSU-INPE-MCT-BR |
Affiliation | 1 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 Name | AGU Chapman Conference: Corotating Solar Wind Streams and Recurrent Geomagnetic Activity. |
Conference Location | Manaus |
Date | 6 a 12 de fevereiro |
Book Title | Anales |
Tertiary Type | Sessão 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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Abstract | During 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. |
Area | CEA |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Determination of Cir... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Determination of Cir... |
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-m13@80/2005/10.13.20.13 |
zipped data URL | http://urlib.net/zip/sid.inpe.br/MTC-m13@80/2005/10.13.20.13 |
Language | en |
Target File | determination cir.pdf |
User Group | administrator marciana seeger05 |
Visibility | shown |
Copy Holder | SID/SCD |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 2 |
Dissemination | <E> |
Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
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6. Notes | |
Empty Fields | archivingpolicy archivist 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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7. Description control | |
e-Mail (login) | marciana |
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