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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/4878D2L
Repositóriosid.inpe.br/mtc-m21d/2022/12.13.17.36
Repositório de Metadadossid.inpe.br/mtc-m21d/2022/12.13.17.36.48
Última Atualização dos Metadados2023:01.03.16.46.27 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoDeggeroniSilvSilvMarc:2022:CaSt
TítuloThe role of the whistler-mode chorus waves in the relativistic electron flux variability of the outer radiation belt under the influence of Coronal Mass Ejection: a case study
Ano2022
Data de Acesso13 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Deggeroni, Vinicius
2 Silva, Ligia Alves da
3 Silva, Marlos Rockenbach da
4 Marchezi, José Paulo
Grupo1 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
3 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Chinese Academy of Sciences
Endereço de e-Mail do Autor1 vinidegg@gmail.com
2 ligia.alves01@gmail.com
3 marlosrs@gmail.com
Nome do EventoAGU Fall Meeting
Localização do EventoChicago, IL
Data12-16 Dec. 2022
Editora (Publisher)AGU
Histórico (UTC)2022-12-13 17:36:48 :: simone -> administrator ::
2023-01-03 16:46:27 :: administrator -> simone :: 2022
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoThe dynamic of Earth's magnetosphere can be disturbed by solar wind structures, such as Coronal Mass Ejection - CME, and change the dynamic of the outer and inner magnetosphere. Those perturbations can generate waves in a wide frequency range, such as whistler-mode chorus waves (from hundreds of Hz up to tens kHz), which can be observed almost simultaneously with the arrival of solar wind structures in the magnetosphere. It means that the trapped particles' dynamic in the outer radiation belt can be violated, causing a direct impact on the population of the outer radiation belt, which is formed primarily by electrons. This impact may occur from different dynamic mechanisms, such as radial diffusion, pitch-angle scattering, magnetopause shadowing, and others. The main goal of this case study, which occurred on October 12, 2012, is to identify the pitch-angle scattering mechanism from the resonance between chorus and relativistic electrons using the Van Allen probes and ACE satellite data. The outer radiation belt's electron flux enhancement (flux increase) and dropout (flux decrease) are analyzed from the characterization of the wave packets (sub-elements) and the calculation of the Wave Normal Angle (WNA) during the influence of a CME. Therefore, this work will characterize the wave's sub-elements during the dropout and enhancement of the outer radiation belt to identify the main differences in the physical processes responsible for the high-energy electron flux variability in the outer radiation belt.
ÁreaCEA
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4. Condições de acesso e uso
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Visibilidadeshown
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5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3F2PBEE
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Acervo Hospedeirourlib.net/www/2021/06.04.03.40
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
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