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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4878CR8
Repositorysid.inpe.br/mtc-m21d/2022/12.13.17.34
Metadata Repositorysid.inpe.br/mtc-m21d/2022/12.13.17.34.33
Metadata Last Update2023:01.03.16.46.27 (UTC) administrator
Secondary KeyINPE--PRE/
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
Access Date2024, Apr. 29
Secondary TypePRE CI
2. Context
Author 1 Marchezi, José Paulo
 2 Dai, Lei
 3 Alves, Livia Ribeiro
 4 Silva, Ligia Alves da
 5 Sibeck, David G.
 6 Dal Lago, Alisson
 7 Souza, Vitor Moura Cardoso e Silva
 8 Jauer, Paulo Ricardo
 9 Vieira, Luís Eduardo Antunes
10 Cardoso, Flávia Regina
11 Deggeroni, Vinicius
12 Alves, Maria Virgínia
13 Wang, Chi
14 Li, Hui
15 Lui, Zhengkuan
Resume Identifier 1
 2
 3
 4
 5
 6 8JMKD3MGP5W/3C9JGH3
 7
 8
 9
10
11
12 8JMKD3MGP5W/3C9JHRS
Group 1
 2
 3 DIHPA-CGCE-INPE-MCTI-GOV-BR
 4
 5
 6 DIHPA-CGCE-INPE-MCTI-GOV-BR
 7 DIHPA-CGCE-INPE-MCTI-GOV-BR
 8 DICEP-CGCE-INPE-MCTI-GOV-BR
 9 DIHPA-CGCE-INPE-MCTI-GOV-BR
10
11 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR
Affiliation 1 Chinese Academy of Sciences
 2 Center for Space Science and Applied Research (CSSAR)
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Chinese Academy of Sciences
 5 NASA/GSFC
 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 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 CSSAR
14 NSSC National Space Science Center
15 NSSC National Space Science Center
Author e-Mail Address 1
 2
 3 livia.alves@inpe.br
 4
 5
 6 alisson.dallago@inpe.br
 7 vitormoura21@gmail.com
 8 pauloricardojauer@gmail.com
 9 luis.vieira71@googlemail.com
10
11 vinidegg@gmail.com
Conference NameAGU Fall Meeting
Conference LocationChicago, IL
Date12-16 Dec. 2022
PublisherAGU
History (UTC)2022-12-13 17:34:33 :: simone -> administrator ::
2022-12-17 09:22:49 :: administrator -> simone :: 2022
2022-12-20 12:07:36 :: simone -> administrator :: 2022
2023-01-03 16:46:27 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
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Transferable1
Content TypeExternal Contribution
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
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