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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/47A6Q2B
Repositorysid.inpe.br/mtc-m21d/2022/07.18.17.57
Last Update2022:07.18.17.57.34 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/07.18.17.57.34
Metadata Last Update2023:01.03.16.46.10 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeySilvaSMSAVADRCWMLJIZ:2022:HiElFl
TitleHigh-energy electron flux enhancement pattern in the outer radiation belt in response to the coronal mass ejections
FormatOn-line
Year2022
Access Date2024, May 14
Secondary TypePRE CI
Number of Files1
Size50 KiB
2. Context
Author 1 Silva, Ligia Alves da
 2 Shi, Jiankui
 3 Marchezi, José Paulo
 4 Sibeck, David
 5 Alves, Livia Ribeiro
 6 Vieira, Luís Eduardo Antunes
 7 Agapitov, Oleksiy
 8 Deggeroni, Vinicius
 9 Resende, Laysa Cristina Araújo
10 Costa, Joaquim Eduardo Rezende
11 Wang, Chi
12 Moro, Juliano
13 Li, Hui
14 Jauer, Paulo Ricardo
15 Inostroza, Ana Maria
16 Zhengkuan, Liu
Resume Identifier 1
 2
 3
 4
 5
 6
 7
 8
 9
10 8JMKD3MGP5W/3C9JHF8
Group 1 DICEP-CGCE-INPE-MCTI-GOV-BR
 2
 3
 4
 5 DIHPA-CGCE-INPE-MCTI-GOV-BR
 6 DIHPA-CGCE-INPE-MCTI-GOV-BR
 7
 8 DIHPA-CGCE-INPE-MCTI-GOV-BR
 9 DICEP-CGCE-INPE-MCTI-GOV-BR
10 DICEP-CGCE-INPE-MCTI-GOV-BR
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12 COESU-CGGO-INPE-MCTI-GOV-BR
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14 DICEP-CGCE-INPE-MCTI-GOV-BR
15 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Chinese Academy of Sciences (CAS)
 3 Chinese Academy of Sciences (CAS)
 4 NASA GSFC
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 UC Berkeley
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Chinese Academy of Sciences (CAS)
14 Instituto Nacional de Pesquisas Espaciais (INPE)
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16 Chinese Academy of Sciences (CAS)
Author e-Mail Address 1 ligia.alves01@gmail.com
 2 jkshi@nssc.ac.cn
 3 jpmarchezi@gmail.com
 4 david.g.sibeck@nasa.gov
 5 liviarib@gmail.com
 6 luis.vieira@inpe.br
 7 agapitov@ssl.berkeley.edu
 8 vinidegg@gmail.com
 9 laysa.resende@gmail.com
10 joaquim.costa@inpe.br
11 cw@spaceweather.ac.cn
12 juliano.moro@inpe.br
13 hli@spaceweather.ac.cn
14 pauloricardojauer@gmail.com
15 anamariainostrozalara@gmail.com
16 liuzhengkuan@nssc.ac.cn
Conference NameCOSPAR Scientific Assembly, 44
Conference LocationAthens, Greece
Date16-24 July 2022
History (UTC)2022-07-18 17:57:34 :: simone -> administrator ::
2022-08-29 18:30:51 :: administrator -> simone :: 2022
2022-12-20 12:11:20 :: simone -> administrator :: 2022
2023-01-03 16:46:10 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe consider the high-energy electron flux enhancements that occur in the outer radiation belt in response to Interplanetary Coronal Mass Ejections (ICMEs). We selected ten events during the Van Allen Probes era in which the high-energy electron flux enhancements start at L-shells below 3.8. Although the physical processes responsible for high-energy electron flux enhancements in the outer radiation belt are known to be associated with the dynamics of the incident solar wind structures and interplanetary transients, there are still several open questions. This work seeks to identify the sequence of ideal physical processes needed for highenergy electron flux enhancements that occur under the influence of the ICMEs via an epoch analysis applied to the interplanetary medium parameters that define ICMEs. Additionally, the dynamic mechanisms driven by both whistler-mode chorus and ultra low-frequency waves will be discussed individually and through epoch analyses to identify the role of these waves in the electron flux enhancement pattern. Thereby, the results of this work may offer support models for the radiation belts within the inner magnetosphere.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > High-energy electron flux...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > High-energy electron flux...
Arrangement 3urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGGO > High-energy electron flux...
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/47A6Q2B
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47A6Q2B
Languageen
Target FilePRBEM.3-0016-22-oral.pdf
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Reader Groupadministrator
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Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2PBEE
8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUBT5
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.22.35 8
sid.inpe.br/mtc-m21/2012/07.13.14.51.06 2
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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