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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3RPHFE5
Repositorysid.inpe.br/mtc-m21c/2018/09.05.11.11
Last Update2018:09.05.11.11.10 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2018/09.05.11.11.10
Metadata Last Update2019:01.14.17.06.34 (UTC) administrator
DOI10.3847/1538-4357/aacdfe
ISSN0004-637X
1538-4357
Citation KeyMunakataKEKKTSDMBSJSDHSK:2018:CoShBu
TitleCosmic-Ray Short Burst Observed with the Global Muon Detector Network (GMDN) on 2015 June 22
Year2018
MonthAug.
Access Date2024, May 18
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2387 KiB
2. Context
Author 1 Munakata, K.
 2 Kozai, M.
 3 Evenson, Paul
 4 Kuwabara, T.
 5 Kato, C.
 6 Tokumaru, Munetoshi
 7 Silva, Marlos Rockenbach da
 8 Dal Lago, Alisson
 9 Mendonça, Rafael Rodrigues Souza de
10 Braga, Carlos Roberto
11 Schuch, Nelson Jorge
12 Jassar, H. K. Al
13 Sharma, M. M.
14 Duldig, M. L.
15 Humble, J. E.
16 Sabbah, I.
17 Kóta, J.
Resume Identifier 1
 2
 3
 4
 5
 6
 7
 8 8JMKD3MGP5W/3C9JGH3
 9
10
11 8JMKD3MGP5W/3C9JHUD
ORCID 1 0000-0002-2131-4100
 2
 3 0000-0001-7929-810X
 4
 5
 6 0000-0002-2982-1887
 7
 8 0000-0002-4361-6492
 9 0000-0002-0417-6877
10
11 0000-0002-7720-6491
Group 1
 2
 3
 4
 5
 6
 7 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 8 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
 9 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
10 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
11 CRCRS-COCRE-INPE-MCTIC-GOV-BR
Affiliation 1 Shinshu University
 2 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA)
 3 University of Delaware
 4 University of Delaware
 5 Shinshu University
 6 Nagoya University
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Kuwait University
13 Kuwait University
14 University of Tasmania
15 University of Tasmania
16 College of Health Sciences, Public Authority of Applied Education and Training, Kuwait City
17 University of Arizona
Author e-Mail Address 1
 2
 3
 4
 5
 6
 7 marlos.silva@inpe.br
 8 alisson.dallago@inpe.br
 9 rafael.mendonca@inpe.br
10 carlos.braga@inpe.br
11 nelson.schuch@inpe.br
JournalAstrophysical Journal
Volume862
Number2
Pagese170
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
History (UTC)2018-09-05 11:11:11 :: simone -> administrator ::
2018-09-05 11:11:11 :: administrator -> simone :: 2018
2018-09-05 11:17:55 :: simone -> administrator :: 2018
2019-01-14 17:06:34 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordscosmic rays
interplanetary medium
Sun: coronal mass ejections (CMEs)
AbstractWe analyze the short cosmic-ray intensity increase ("cosmic-ray burst": CRB) on 2015 June 22 utilizing a global network of muon detectors and derive the global anisotropy of cosmic-ray intensity and the density (i.e., the omnidirectional intensity) with 10 minute time resolution. We find that the CRB was caused by a local density maximum and an enhanced anisotropy of cosmic rays, both of which appeared in association with Earth's crossing of the heliospheric current sheet (HCS). This enhanced anisotropy was normal to the HCS and consistent with a diamagnetic drift arising from the spatial gradient of cosmic-ray density, which indicates that cosmic rays were drifting along the HCS from the north of Earth. We also find a significant anisotropy along the HCS, lasting a few hours after the HCS crossing, indicating that cosmic rays penetrated into the inner heliosphere along the HCS. Based on the latest geomagnetic field model, we quantitatively evaluate the reduction of the geomagnetic cutoff rigidity and the variation of the asymptotic viewing direction of cosmic rays due to a major geomagnetic storm that occurred during the CRB and conclude that the CRB is not caused by the geomagnetic storm, but by a rapid change in the cosmic-ray anisotropy and density outside the magnetosphere.
AreaCEA
Arrangement 1urlib.net > Produção anterior à 2021 > DIDGE > Cosmic-Ray Short Burst...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Cosmic-Ray Short Burst...
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4. Conditions of access and use
data URLhttp://mtc-m21c.sid.inpe.br/ibi/8JMKD3MGP3W34R/3RPHFE5
zipped data URLhttp://mtc-m21c.sid.inpe.br/zip/8JMKD3MGP3W34R/3RPHFE5
Languageen
Target Filemunakata_cosmic.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.39.46 4
sid.inpe.br/mtc-m21/2012/07.13.14.57.02 2
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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