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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47S4LBE
Repositorysid.inpe.br/mtc-m21d/2022/10.24.16.14   (restricted access)
Last Update2022:10.24.16.14.56 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/10.24.16.14.56
Metadata Last Update2023:01.23.17.06.34 (UTC) administrator
DOI10.3389/fspas.2022.970308
ISSN2296-987X
Citation KeySilvaSRAABAVDMWMILMCJACLDG:2022:RoInRa
TitleThe role of the inner radiation belt dynamic in the generation of auroral-type sporadic E-layers over south American magnetic anomaly
Year2022
MonthSept.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size6871 KiB
2. Context
Author 1 Silva, Ligia Alves da
 2 Shi, J.
 3 Resende, Laysa Cristina Araújo
 4 Agapitov, O. V.
 5 Alves, Livia Ribeiro
 6 Batista, Inez Staciarini
 7 Arras, C.
 8 Vieira, Luís Eduardo Antunes
 9 Deggeroni, Vinícius
10 Marchezi, José Paulo
11 Wang, C.
12 Moro, Juliano
13 Inostroza, A.
14 Li, H.
15 Medeiros, Cláudia
16 Cardoso, F. R.
17 Jauer, Paulo Ricardo
18 Alves, Maria Virgínia
19 Chen, Sony Su
20 Liu, Z.
21 Denardini, Clezio Marcos
22 Gonzalez Alarcon, Walter Demetrio
Resume Identifier 1
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 6 8JMKD3MGP5W/3C9JHDA
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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 University of California Berkeley
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 German Research Centre for Geosciences
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Chinese Academy of Sciences
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Instituto Nacional de Pesquisas Espaciais (INPE)
14 Chinese Academy of Sciences
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16 Universidade de São Paulo (SP)
17 Instituto Nacional de Pesquisas Espaciais (INPE)
18 Instituto Nacional de Pesquisas Espaciais (INPE)
19 Instituto Nacional de Pesquisas Espaciais (INPE)
20 Chinese Academy of Sciences
21 Instituto Nacional de Pesquisas Espaciais (INPE)
22 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 ligia.alves01@gmail.com
 2
 3 laysa.resende@gmail.com
 4
 5 livia.alves@inpe.br
 6 staciarinibatista.inez@gmail.com
 7
 8 luis.vieira71@googlemail.com
 9 vinidegg@gmail.com
10 jpmarchezi@gmail.com
11
12 julianopmoro@gmail.com
13
14
15 claudia.inpe@gmail.com
16
17 pauloricardojauer@gmail.com
18
19 sony.chen@inpe.br
20
21 clezio.denardin@inpe.br
22 walterdgalarcon@yahoo.com
JournalFrontiers in Astronomy and Space Sciences
Volume9
Pagese970308
History (UTC)2022-10-24 16:18:12 :: simone -> administrator :: 2022
2022-11-01 05:59:21 :: administrator -> simone :: 2022
2022-12-20 11:40:23 :: simone -> administrator :: 2022
2023-01-23 17:06:34 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsauroral-type sporadic E-layers
hiss waves
inner radiation belt
ionosphere
magnetosonic waves
South American Magnetic Anomaly
wave-particle interaction
AbstractThe dynamics of the electron population in the Earths radiation belts affect the upper atmospheres ionization level through the low-energy Electron Precipitation (EP). The impact of low-energy EP on the high-latitude ionosphere has been well explained since the 1960s decade. Conversely, it is still not well understood for the region of the South American Magnetic Anomaly (SAMA). In this study, we present the results of analysis of the strong geomagnetic storm associated with the Interplanetary Coronal Mass Ejection (May 27-28, 2017). The atypical auroral sporadic E layers (Esa) over SAMA are observed in concomitance with the hiss and magnetosonic wave activities in the inner radiation belt. The wave-particle interaction effects have been estimated, and the dynamic mechanisms that caused the low-energy EP over SAMA were investigated. We suggested that the enhancement in pitch angle scattering driven by hiss waves result in the low-energy EP (≥10 keV) into the atmosphere over SAMA. The impact of these precipitations on the ionization rate at the altitude range from 100 to 120 km can generate the Esa layer in this peculiar region. In contrast, we suggested that the low-energy EP (≤1 keV) causes the maximum ionization rate close to 150 km altitude, contributing to the Esa layer occurrence in these altitudes.
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Languageen
Target Filefspas-09-970308.pdf
User Groupsimone
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Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2PBEE
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Citing Item Listsid.inpe.br/bibdigital/2022/04.03.23.11 3
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 3
sid.inpe.br/bibdigital/2013/10.12.21.02 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
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