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1. Identity statement
Reference TypeConference Abstract (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/38TT6M2
Repositorysid.inpe.br/mtc-m19/2011/01.08.23.51   (restricted access)
Last Update2011:01.08.23.51.16 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/01.08.23.51.15
Metadata Last Update2018:06.05.04.35.08 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyKemerichLSSVBSS:2010:AnObBr
TitleAnisotropy Observed at the Brazilian Southern Space Observatory by the Multidirectional Muon Detector MMD
Year2010
Access Date2024, Apr. 28
Secondary TypePRE CI
Number of Files1
Size33 KiB
2. Context
Author1 Kemerich, Nikolas
2 Lago, Alisson Dal
3 Schuch, Nelson Jorge
4 Silva, Marlos Rockenbach da
5 Viera, L. R.
6 Braga, Carlos Roberto
7 Silveira, Marcos Vinicius Dias da
8 Stekel, Tardelli Ronan Coelho
Resume Identifier1
2 8JMKD3MGP5W/3C9JGH3
3 8JMKD3MGP5W/3C9JHUD
Group1
2 DGE-CEA-INPE-MCT-BR
3 CRS-CCR-INPE-MCT-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference Name38th COSPAR Scientific Assembly
Conference LocationBremen, Alemanha
Date18-25 July
Book TitleAbstracts
History (UTC)2011-01-08 23:51:43 :: seeger05 -> administrator :: 2010
2018-06-05 04:35:08 :: administrator -> seeger05 :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractGalactic Cosmic Rays (GCR) (~50 GeV) are observed by ground-level detectors. They suffer modulation effects due to interplanetary disturbances such as ICMEs and its correspondent structures, i.e., interplanetary shock waves and magnetic clouds which can cause geomagnetic storms in the Earths magnetosphere. Forbush Decrease (FD) is an intense decrease of cosmic rays formed behind the shock accompanied by an ICME. Certain kinds of decreases were observed before a FD, and they are precursory anisotropy seen like kinetic effects related with the interaction of cosmic rays and the upstream of the approaching shock in the interplanetary medium. This work discusses the possibility of Space Weather forecasting using ground-based multidirectional muon detector to identify precursory anisotropy in the interplanetary medium. Data of plasma parameters and magnetic field from Advanced Composition Explorer (ACE) satellite and Dst index are used for comparison with the cosmic rays data to identify the structures at the solar wind and to recognizing geomagnetic storms occurred in the Earths magnetosphere. The prototype detector of secondary cosmic rays, muons, was installed at the Southern Space Observatory SSO/CRS/INPE MCT (29.4ºS, 53.8° W, 480 m ) in 2001, São Martinho da Serra, RS, in South of Brazil and this detector was upgraded in 2005. Decreases in intensity of muons before the passage of an ICME in the earth are expected to be observed. The cosmic ray detector at SSO is important part of Global Muon Detector Network GMDN.
AreaCEA
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4. Conditions of access and use
Languageen
Target FileCOSPAR 2010 Abstract Nikolas Kemmerich.pdf
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seeger05
Visibilityshown
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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