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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
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Identifier8JMKD3MGP3W34T/47H65RE
Repositorysid.inpe.br/mtc-m21d/2022/08.30.15.38
Last Update2022:08.30.15.38.43 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21d/2022/08.30.15.38.43
Metadata Last Update2023:02.03.14.33.07 (UTC) administrator
DOI10.1029/2021JA029887
ISSN2169-9402
Citation KeyMarcheziDASSDSJVCDAWLL:2022:StAnVa
TitleElectron Flux Variability and Ultra-Low Frequency Wave Activity in the Outer Radiation Belt Under the Influence of Interplanetary Coronal Mass Ejections and High-Speed Solar Wind Streams: A Statistical Analysis From the Van Allen Probes Era
Year2022
MonthAug.
Access Date2024, Apr. 29
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3734 KiB
2. Context
Author 1 Marchezi, José Paulo
 2 Dai, L.
 3 Alves, Livia Ribeiro
 4 Silva, Ligia Alves da
 5 Sibeck, D. G.
 6 Dal Lago, Alisson
 7 Souza, Vitor Moura Cardoso e Silva
 8 Jauer, Paulo Ricardo
 9 Vieira, Luís Eduardo Antunes
10 Cardoso, F. R.
11 Deggeroni, Vinícius
12 Alves, Maria Virgínia
13 Wang, C.
14 Li, H.
15 Liu, Z.
Resume Identifier 1
 2
 3
 4
 5
 6 8JMKD3MGP5W/3C9JGH3
 7
 8
 9
10
11
12 8JMKD3MGP5W/3C9JHRS
ORCID 1 0000-0002-2904-6411
 2 0000-0002-5122-3066
 3 0000-0002-5680-7271
 4 0000-0002-8822-5030
 5 0000-0003-3240-7510
 6 0000-0002-4361-6492
 7 0000-0001-7294-7963
 8 0000-0002-8064-5030
 9 0000-0002-9376-475X
10 0000-0001-7239-0894
11 0000-0002-0725-6055
12
13 0000-0001-6991-9398
Group 1
 2
 3 DIHPA-CGCE-INPE-MCTI-GOV-BR
 4 DIHPA-CGCE-INPE-MCTI-GOV-BR
 5
 6 DIHPA-CGCE-INPE-MCTI-GOV-BR
 7 YYY-CGCE-INPE-MCTI-GOV-BR
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 9 DIHPA-CGCE-INPE-MCTI-GOV-BR
10
11 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR
12 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Chinese Academy of Sciences (CAS)
 2 Chinese Academy of Sciences (CAS)
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 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 Universidade de São Paulo (USP)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Chinese Academy of Sciences (CAS)
14 Chinese Academy of Sciences (CAS)
15 Chinese Academy of Sciences (CAS)
Author e-Mail Address 1 jpmarchezi@gmail.com
 2
 3 livia.alves@inpe.br
 4 ligia.alves01@gmail.com
 5
 6 alisson.dallago@inpe.br
 7 vitormoura21@gmail.com
 8 pauloricardojauer@gmail.com
 9 luis.vieira71@googlemail.com
10
11 vinidegg@gmail.com
JournalJournal of Geophysical Research - Space Physics
Volume127
Number8
Pagese2021JA029887
History (UTC)2022-08-30 15:38:43 :: simone -> administrator ::
2022-08-30 15:38:44 :: administrator -> simone :: 2022
2022-08-30 15:40:00 :: simone -> administrator :: 2022
2022-09-01 23:17:29 :: administrator -> simone :: 2022
2022-12-20 12:07:07 :: simone -> administrator :: 2022
2023-02-03 14:33:07 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsULF waves
depletions
enhancement
radiation belts
alfven waves
geomagnetic pulsations
AbstractThe ultra-low frequency (ULF) waves can stochastically accelerate radiation belt electrons. Radial diffusion is a well-established mechanism that can enhance or reduce the electron population in combination with other processes. Using data from the Van Allen Probes, we investigated the response of the 2.10 MeV energy electrons and ULF waves to two types of solar wind structures interacting with Earth's magnetosphere, namely, interplanetary coronal mass ejections (ICMEs) and High-Speed solar wind streams (HSS). We use measured electron differential flux and ULF waves in the Pc4-Pc5 frequency range from October 2012 to May 2019. We examine 155 events with changes in the outer radiation belt electron differential flux. Results considering all ICMEs and HSSs during the Van Allen Probes era show that for both solar wind structures, solar wind interplanetary magnetic field Bz, solar wind proton density, and speed are related to the outer radiation belt relativistic electrons' response. The persistent ULF power is present during enhancement cases, while for reduction, the ULF waves power is concentrated at the initial reduction on the outer radiation belt electron flux.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Electron Flux Variability...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34T/47H65RE
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34T/47H65RE
Languageen
Target FileJGR Space Physics - 2022 - Marchezi - Electron Flux Variability and Ultra‐Low Frequency Wave Activity in the Outer.pdf
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Update Permissionnot transferred
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Next Higher Units8JMKD3MGPCW/3F2PBEE
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DisseminationWEBSCI; PORTALCAPES; AGU.
Host Collectionurlib.net/www/2021/06.04.03.40
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