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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/45D52JB
Repositorysid.inpe.br/mtc-m21d/2021/09.07.15.24
Last Update2021:09.07.15.24.34 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21d/2021/09.07.15.24.34
Metadata Last Update2022:04.03.19.24.01 (UTC) administrator
DOI10.1029/2021JA029363
ISSN2169-9402
Citation KeySilvaSASMMVACSDJWLLAS:2021:StAn
TitleHigh-Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to the Alfvénic Fluctuations Within High-Speed Solar Wind Stream: A Statistical Analysis
Year2021
MonthAug.
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size9474 KiB
2. Context
Author 1 Silva, Ligia Alves da
 2 Shi, J.
 3 Alves, Livia Ribeiro
 4 Sibeck, D.
 5 Marchezi, José Paulo
 6 Medeiros, Cláudia
 7 Vieira, Luís Eduardo Antunes
 8 Agapitov, O.
 9 Cardoso, F. R.
10 Souza, Vitor Moura Cardoso e Silva
11 Dal Lago, Alisson
12 Jauer, Paulo Roberto
13 Wang, C.
14 Li, H.
15 Liu, Z.
16 Alves, Maria Virgínia
17 Silva, Marlos Rockenbach da
Resume Identifier 1
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ORCID 1 0000-0002-8822-5030
 2 0000-0002-8008-0527
 3 0000-0002-5680-7271
 4 0000-0003-3240-7510
 5 0000-0002-2904-6411
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Group 1 DIHPA-CGCE-INPE-MCTI-GOV-BR
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 3 DIHPA-CGCE-INPE-MCTI-GOV-BR
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 5 DIHPA-CGCE-INPE-MCTI-GOV-BR
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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 University of California
 9 Universidade de São Paulo (USP)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Chinese Academy of Sciences
14 Chinese Academy of Sciences
15 Chinese Academy of Sciences
16 Instituto Nacional de Pesquisas Espaciais (INPE)
17 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 ligia.alves01@gmail.com
JournalJournal of Geophysical Research: Space Physics
Volume126
Number8
Pagese2021JA029363
History (UTC)2021-09-07 15:24:34 :: simone -> administrator ::
2021-09-07 15:24:35 :: administrator -> simone :: 2021
2021-09-07 15:30:32 :: simone -> administrator :: 2021
2022-04-03 19:24:01 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordselectron flux enhancement
high speed solar wind stream
high-energy electron flux
outer radiation belt
ultra low frequency waves
whistler-mode chorus waves
AbstractThe coupling response between solar wind structures and the magnetosphere is highly complex, leading to different effects in the outer radiation belt electron fluxes. Most Coronal Mass Ejections cause strong geomagnetic storms with short recovery phases, often 12 days. By contrast, High-Speed Solar Wind Streams lead to moderate and weak storms often with much longer recovery phases, from several to ∼10 days. The magnetosphere receives energy for a long time under the influence of the HSSs, considerably changing its dynamics. This in turn has an effect on the charged particles trapped in the outer radiation belt. Although the high-energy electron flux enhancements have received considerable attention, the high-energy electron flux enhancement pattern (L > 4) has not. This paper identifies 37 events with this enhancement pattern in the high-energy electron flux during the Van Allen Probes era. We find the enhancements coincident with HSS occurrence. The interplanetary magnetic field (IMF) exhibits north/south Bz fluctuations of Alfvénic nature with moderate amplitudes. The high-energy electron flux enhancements also correspond to long periods of auroral activity indicating a relationship to magnetotail dynamics. However, the AE index only reaches moderate values. Ultra-Low Frequency waves were present in all of the events and whistler-mode chorus waves were present in 89.1% of the events, providing a convenient scenario for wave-particle interactions. The radial gradient of the ULF wave power related to the L, under the influence of the HSSs, is necessary to trigger the physical processes responsible for this type of high-energy electron flux enhancement pattern.
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Languageen
Target Filesilva_high.pdf
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Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.55.54 5
sid.inpe.br/mtc-m21/2012/07.13.14.39.46 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
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