Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44JA9AB
Repositorysid.inpe.br/mtc-m21c/2021/04.26.12.24   (restricted access)
Last Update2021:04.26.12.24.43 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2021/04.26.12.24.44
Metadata Last Update2022:04.03.22.39.37 (UTC) administrator
DOI10.1029/2020SW002531
ISSN1539-4956
Citation KeyKiharaMKKKMKKTMEDSSBBASDHESK:2021:PeICEv
TitleA Peculiar ICME Event in August 2018 Observed With the Global Muon Detector Network
Year2021
MonthMar.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1241 KiB
2. Context
Author 1 Kihara, W.
 2 Munakata, K.
 3 Kato, C.
 4 Kataoka, R.
 5 Kadokura, A.
 6 Miyake, S.
 7 Kozai, M.
 8 Kuwabara, T.
 9 Tokumaru, M.
10 Mendonça, R. R. S.
11 Echer, Ezequiel
12 Dal Lago, Alisson
13 Silva, Marlos Rockenbach da
14 Schuch, Nelson Jorge
15 Bageston, José Valentin
16 Braga, C. R.
17 Al Jassar, H. K.
18 Sharma, M. M.
19 Duldig, M. L.
20 Humble, J. E.
21 Evenson, P.
22 Sabbah, I.
23 Kóta, J.
Resume Identifier 1
 2
 3
 4
 5
 6
 7
 8
 9
10
11 8JMKD3MGP5W/3C9JH3D
12 8JMKD3MGP5W/3C9JGH3
13
14 8JMKD3MGP5W/3C9JHUD
ORCID 1 0000-0003-1367-0727
 2 0000-0002-2131-4100
 3 0000-0002-4913-8225
 4 0000-0001-9400-1765
 5 0000-0002-6105-9562
 6 0000-0002-3067-655X
 7 0000-0002-3948-3666
 8 0000-0001-6584-9054
 9 0000-0002-2982-1887
10 0000-0002-0417-6877
11 0000-0002-8351-6779
12 0000-0002-4361-6492
13 0000-0002-9737-9429
14 0000-0002-7720-6491
15 0000-0003-2931-8488
16 0000-0003-1485-9564
17 0000-0002-4486-237X
18
19 0000-0001-7463-8267
20 0000-0002-4698-1671
21 0000-0001-7929-810X
22 0000-0002-7037-322X
23 0000-0002-3715-0358
Group 1
 2
 3
 4
 5
 6
 7
 8
 9
10 GES-CEA-DIPGR-INPE-MCTI-GOV-BR
11 DIHPA-CGCE-INPE-MCTI-GOV-BR
12 DIHPA-CGCE-INPE-MCTI-GOV-BR
13 DIHPA-CGCE-INPE-MCTI-GOV-BR
14 COESU-CGGO-INPE-MCTI-GOV-BR
15 COESU-CGGO-INPE-MCTI-GOV-BR
Affiliation 1 Shinshu University
 2 Shinshu University
 3 Shinshu University
 4 National Institute of Polar Research
 5 National Institute of Polar Research
 6 National Institute of Technology
 7 Japan Aerospace Exploration Agency
 8 Chiba University
 9 Nagoya University
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Instituto Nacional de Pesquisas Espaciais (INPE)
14 Instituto Nacional de Pesquisas Espaciais (INPE)
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16 George Mason University
17 Kuwait University
18 Kuwait University
19 University of Tasmania
20 University of Tasmania
21 University of Delaware
22 College of Technological Studies
23 University of Arizona
Author e-Mail Address 1 19ss204g@shinshu-u.ac.jp
 2
 3
 4
 5
 6
 7
 8
 9
10
11 ezequiel.echer@gmail.com
12 alisson.dallago@inpe.br
13 marlosrs@gmail.com
14 njschuch@gmail.com
15 jose.bageston@inpe.br
JournalSpace Weather
Volume19
Number3
Pagese2020W002531
History (UTC)2021-04-26 12:24:44 :: simone -> administrator ::
2021-04-26 12:24:45 :: administrator -> simone :: 2021
2021-04-26 12:27:33 :: simone -> administrator :: 2021
2022-04-03 22:39:37 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordscoronal mass ejection
corotating interaction region
cosmic‐

ray
geomagnetic storm
magnetic flux rope
solar minimum
AbstractWe demonstrate that global observations of high-energy cosmic rays contribute to understanding unique characteristics of a large-scale magnetic flux rope causing a magnetic storm in August 2018. Following a weak interplanetary shock on August 25, 2018, a magnetic flux rope caused an unexpectedly large geomagnetic storm. It is likely that this event became geoeffective because the flux rope was accompanied by a corotating interaction region and compressed by high-speed solar wind following the flux rope. In fact, a Forbush decrease was observed in cosmic-ray data inside the flux rope as expected, and a significant cosmic-ray density increase exceeding the unmodulated level before the shock was also observed near the trailing edge of the flux rope. The cosmic-ray density increase can be interpreted in terms of the adiabatic heating of cosmic rays near the trailing edge of the flux rope, as the corotating interaction region prevents free expansion of the flux rope and results in the compression near the trailing edge. A northeast-directed spatial gradient in the cosmic-ray density was also derived during the cosmic-ray density increase, suggesting that the center of the heating near the trailing edge is located northeast of Earth. This is one of the best examples demonstrating that the observation of high-energy cosmic rays provides us with information that can only be derived from the cosmic ray measurements to observationally constrain the three-dimensional macroscopic picture of the interaction between coronal mass ejections and the ambient solar wind, which is essential for prediction of large magnetic storms.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > A Peculiar ICME...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > A Peculiar ICME...
Arrangement 3urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGGO > A Peculiar ICME...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 26/04/2021 09:24 1.0 KiB 
4. Conditions of access and use
Languageen
Target Filekihara_peculiar.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2PBEE
8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUBT5
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.39.46 5
sid.inpe.br/bibdigital/2022/04.03.22.35 3
sid.inpe.br/mtc-m21/2012/07.13.14.57.02 2
DisseminationWEBSCI
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Description control
e-Mail (login)simone
update 


Close