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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4A7L7MB
Repositorysid.inpe.br/mtc-m21d/2023/11.13.13.45
Last Update2023:11.13.13.45.51 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21d/2023/11.13.13.45.51
Metadata Last Update2024:05.02.18.31.39 (UTC) administrator
DOI10.1029/2023JA031360
ISSN2169-9402
Labelself-archiving-INPE-MCTIC-GOV-BR
Citation KeySilvaSMASAVDRLCWMLDFIL:2023:HiElFl
TitleHigh-Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to the Interplanetary Coronal Mass Ejections
Year2023
MonthNov.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3843 KiB
2. Context
Author 1 Silva, Ligia Alves da
 2 Shi, J.
 3 Marchezi, J. P.
 4 Agapitov, O. V.
 5 Sibeck, D.
 6 Alves, Livia Ribeiro
 7 Vieira, Luis Eduardo Antunes
 8 Deggeroni, Vinicius
 9 Resende, Laysa Cristina Araújo
10 Lopez, F.
11 Costa, Joaquim Eduardo Rezende
12 Wang, C.
13 Moro, Juliano
14 Li, H.
15 Dal Lago, Alisson
16 Ferreira, Karen Júlia Coldebella
17 Inostroza Lara, Ana Maria
18 Liu, Z.
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11 8JMKD3MGP5W/3C9JHF8
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ORCID 1 0000-0002-8822-5030
 2
 3 0000-0002-2904-6411
 4 0000-0001-6427-1596
 5 0000-0003-3240-7510
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Group 1 DIHPA-CGCE-INPE-MCTI-GOV-BR
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Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Chinese Academy of Sciences
 3 University of New Hampshire
 4 University of California
 5 NASA Goddard Space Flight Center
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 The University of Texas
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Chinese Academy of Sciences
13 Instituto Nacional de Pesquisas Espaciais (INPE)
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 Chinese Academy of Sciences
Author e-Mail Address 1 ligia.alves01@gmail.com
 2
 3
 4
 5
 6 livia.alves@inpe.br
 7 luis.vieira@inpe.br
 8 vinicius.deggeroni@inpe.br
 9 laysa.resende@inpe.br
10
11 joaquim.costa@inpe.br
12
13 juliano.moro@inpe.br
14
15 alisson.dallago@inpe.br
16 karen.ferreira@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume128
Number11
Pagese2023JA031360
History (UTC)2023-11-13 13:45:51 :: simone -> administrator ::
2023-11-13 13:45:58 :: administrator -> simone :: 2023
2023-11-13 13:47:42 :: simone -> administrator :: 2023
2023-12-18 23:44:58 :: administrator -> self-uploading-INPE-MCTI-GOV-BR :: 2023
2023-12-19 02:22:46 :: self-uploading-INPE-MCTI-GOV-BR -> administrator :: 2023
2024-05-02 18:31:39 :: administrator -> simone :: 2023
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe high-energy electron flux enhancement pattern in the outer radiation belt is observed under the influence of the Interplanetary Coronal Mass Ejections (ICMEs). Ten events were selected during the Van Allen Probes era, with the high-energy electron flux enhancement starting close to L* = 4. A schematic diagram of the main physical processes responsible for this kind of high-energy electron flux enhancement is presented, considering the energy deposited in the inner magnetosphere under the influence of ICMEs. Superposed Epoch Analysis is applied to the interplanetary medium parameters, the magnetopause standoff distance, the storm-time geomagnetic activity indices, the Ultra-Low Frequency (ULF) waves, and the whistler-mode chorus waves. A compressed magnetopause, Bz component preferentially southward and storm indices considerably high are observed at the beginning of the electron flux enhancements. The modeled parameters of the chorus waves at the dayside/nightside sectors show the high acceleration efficiency at the beginning of the electron flux enhancement pattern II. These results suggest that the local acceleration driven by chorus waves is essential to these electron flux enhancements at low L*. In contrast, although the ULF waves are detected at the beginning of the studied electron flux enhancements, their contribution is insignificant.
AreaCEA
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Languageen
Target FileJGR Space Physics - 2023 - Silva - High‐Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to.pdf
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Next Higher Units8JMKD3MGPCW/3F2PBEE
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DisseminationWEBSCI; AGU; MGA; COMPENDEX.
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