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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/iris@1916/2006/01.05.16.37   (restricted access)
Last Update2006:01.05.16.37.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2006/01.05.16.37.08
Metadata Last Update2018:06.05.01.16.42 (UTC) administrator
Secondary KeyINPE-13299-PRE/8541
ISSN0273-1177
Citation KeyMunakataKBEPYKFDHTAS:2005:CmCoAn
TitleCme-geometry and cosmic-ray anisotropy observed by a prototype muon
Year2005
Access Date2024, May 18
Secondary TypePRE PI
Number of Files1
Size414 KiB
2. Context
Author 1 Munakata, Kazuoki
 2 Kuwabara, T.
 3 Bieber, J. W.
 4 Evenson, P.
 5 Pyle, R.
 6 Yasue, S.
 7 Kato, C.
 8 Fujii, Z.
 9 Duldig, M. L.
10 Humble, J. E.
11 M. R. Silva
12 Trivedi, Nalin Babulal
13 Alarcon, Walter Demétrio Gonzalez
14 Schuch, Nelson Jorge
Resume Identifier 1
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10
11
12 8JMKD3MGP5W/3C9JHTS
13 8JMKD3MGP5W/3C9JJC4
14 8JMKD3MGP5W/3C9JHUD
Group 1
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11 DGE-INPE-MCT-BR
12 DGE-INPE-MCT-BR
13 DGE-INPE-MCT-BR
14 RSU-INPE-MCT-BR
JournalAdvances in Space Research
Volume36
Pages2357-2362
History (UTC)2006-01-05 17:11:27 :: jefferson -> administrator ::
2008-06-10 22:41:45 :: administrator -> jefferson ::
2008-06-30 18:06:35 :: jefferson -> administrator ::
2012-07-17 12:41:33 :: administrator -> jefferson ::
2012-10-03 14:47:35 :: jefferson -> administrator :: 2005
2018-06-05 01:16:42 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsCoronal mass ejection
forbush decrease
cosmic ray anisotropy
AbstractWe analyze the cosmic-ray anisotropy observed by a prototype network of muon detectors during geomagnetic storms associated with coronal mass ejections (CMEs). The network currently consists of multidirectional surface muon detectors at Nagoya (Japan) and Hobart (Australia), together with a prototype detector at Sao Martinho (Brazil) which has been in operation since March, 2001. In this report, we analyze the anisotropy recorded in both the muon detector and neutron monitor (the Spaceship Earth) networks and find significant enhancements of cosmic-ray anisotropy during geomagnetic storms. Following the analysis by Bieber and Evenson [Bieber, J.W., Evenson, P. CME geometry in relation to cosmic ray anisotropy. Geophys. Res. Lett. 25 (1998) 29552958] for the neutron monitor data at 10 GeV, we also derive cosmic-ray density gradients from muon data at higher-energy (50 GeV), possibly reflecting the larger-scale geometry of CMEs causing geomagnetic storms. We particularly find in some events the anisotropy enhancement clearly starting prior to the storm onset in both the muon and neutron data. This is the first result of the CME-geometry derived from simultaneous observations of the anisotropy with networks of multidirectional muon detectors and neutron monitors. 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.
AreaCEA
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4. Conditions of access and use
Languageen
Target FileCME-geometry and cosmic-ray anisotropy observed by a prototype muon  detector network.pdf
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Archiving Policydenypublisher denyfinaldraft24
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5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/bibdigital/2013/10.04.21.53 2
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 2
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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