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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44BEUL5
Repositorysid.inpe.br/mtc-m21c/2021/03.15.12.50
Last Update2021:03.15.12.50.52 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2021/03.15.12.50.52
Metadata Last Update2022:04.03.23.14.27 (UTC) administrator
DOI10.1029/2020JA028492
ISSN2169-9402
Citation KeySilvaSASSMMVAJAWLLDASBZK:2021:DyMeAs
TitleDynamic Mechanisms Associated With High-Energy Electron Flux Dropout in the Earth's Outer Radiation Belt Under the Influence of a Coronal Mass Ejection Sheath Region
Year2021
MonthJan.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size11896 KiB
2. Context
Author 1 Silva, Ligia Alves da
 2 Shi, Jiankui
 3 Alves, Livia Ribeiro
 4 Sibeck, David G.
 5 Souza, Vitor Moura Cardoso e Silva
 6 Marchezi, José Paulo
 7 Medeiros, Cláudia
 8 Vieira, Luis Eduardo Antunes
 9 Agapitov, Oleksiy
10 Jauer, Paulo R.
11 Alves, M. E. S.
12 Wang, Chi
13 Li, H.
14 Liu, Z.
15 Dal Lago, Alisson
16 Alves, Maria Virginia
17 Silva, Marlos Rockenbach da
18 Baker, Daniel N.
19 Zhang, S. Y.
20 Kenekal, Shrikanth G.
Resume Identifier 1
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15 8JMKD3MGP5W/3C9JGH3
16 8JMKD3MGP5W/3C9JHRS
ORCID 1 0000-0002-8822-5030
 2
 3 0000-0002-5680-7271
 4 0000-0003-3240-7510
 5 0000-0001-7294-7963
 6 0000-0002-2904-6411
 7 0000-0002-6914-5799
 8 0000-0002-9376-475X
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Group 1 DIHPA-CGCE-INPE-MCTI-GOV-BR
 2
 3 DIHPA-CGCE-INPE-MCTI-GOV-BR
 4
 5 DIHPA-CGCE-INPE-MCTI-GOV-BR
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 7 CORCR-CGIP-INPE-MCTI-GOV-BR
 8 DIHPA-CGCE-INPE-MCTI-GOV-BR
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15 DIHPA-CGCE-INPE-MCTI-GOV-BR
16 DIHPA-CGCE-INPE-MCTI-GOV-BR
17 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Chinese Academy of Sciences
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 NASA Goddard Space Flight Center
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 University of California
10 Chinese Academy of Sciences
11 Universidade Estadual Paulista (UNESP)
12 Chinese Academy of Sciences
13 Chinese Academy of Sciences
14 Chinese Academy of Sciences
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16 Instituto Nacional de Pesquisas Espaciais (INPE)
17 Instituto Nacional de Pesquisas Espaciais (INPE)
18 Laboratory for Atmosphere and Space Physics
19 Chinese Academy of Sciences
20 NASA Goddard Space Flight Center
Author e-Mail Address 1 ligia.alves01@gmail.com
 2
 3 livia.alves@inpe.br
 4
 5 vitormoura21@gmail.com
 6 jose.marchezi@inpe.br
 7 claudia.inpe@gmail.com
 8 luis.vieira71@googlemail.com
 9
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15 alisson.dallago@inpe.br
16 ma.alves@inpe.br
17 marlosrs@gmail.com
JournalJournal of Geophysical Research: Space Physics
Volume126
Number1
PageseJGRA56114
History (UTC)2021-03-15 12:50:52 :: simone -> administrator ::
2021-03-15 12:50:53 :: administrator -> simone :: 2021
2021-03-15 12:53:11 :: simone -> administrator :: 2021
2021-06-22 19:11:14 :: administrator -> simone :: 2021
2021-06-22 20:42:38 :: simone -> administrator :: 2021
2022-04-03 23:14:27 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe near-Earth interplanetary environment conditions affect the dynamics of the relativistic electron population quasitrapped in the radiation belts. A complex chain of processes observed in the magnetosphere can contribute to the variability of these populations when interplanetary structures, such as the interplanetary counterpart of a solar coronal mass ejection (ICME), and high-speed solar wind streams interact with the magnetosphere. However, as these processes can coexist, it is hard to untangle the relative contribution of each process to the loss of particles and the eventual repopulation. Here we show evidence that it is possible to distinguish the relative contribution of mechanisms related to the loss of the outer radiation belt electrons for an event observed on July 19 and 20, 2016. The interaction of an ICME's turbulent sheath with the Earth's magnetosphere resulted in a decrease in the outer radiation belt relativistic electron population. The ultralow frequency (ULF) and chorus wave activities are detected in the outer radiation belt during the time when the Earth's magnetosphere is under the influence of the ICME's sheath region, as well as the ICME's magnetic cloud region, while the electromagnetic ion cyclotron (EMIC) waves in the outer belt are observed only during the sheath region. Dynamic mechanisms such as magnetopause shadowing, outward radial diffusion driven by ULF waves, pitch-angle scattering driven by both EMIC and chorus waves are quantitatively analyzed. Our results suggest that the structures of the ICMEs can trigger the drivers to generate the different dynamic mechanisms responsible for the radiation belt population variability.
AreaCEA
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/44BEUL5
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/44BEUL5
Languageen
Target Filesilva_dynamic.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUES5
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.55.54 3
sid.inpe.br/mtc-m21/2012/07.13.14.39.46 2
sid.inpe.br/bibdigital/2022/04.03.23.11 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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