1. Identificação | |
Tipo de Referência | Artigo em Evento (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/44D4NML |
Repositório | sid.inpe.br/mtc-m21c/2021/03.25.12.12 |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2021/03.25.12.12.22 |
Última Atualização dos Metadados | 2022:04.03.23.14.49 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
Chave de Citação | SilvaSSJSMSKBKB:2021:HoDoRe |
Título | How Does Relativistic Outer Radiation Belt Electron Flux Change Under Recurrent Solar Wind Structures? |
Ano | 2021 |
Data de Acesso | 20 maio 2024 |
Tipo Secundário | PRE CN |
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2. Contextualização | |
Autor | 1 Silva, Ligia Alves da 2 Silva, Graziela Belmira Dias da 3 Silva, Ligia Alves da 4 Jauer, Paulo Ricardo 5 Souza, Vitor Moura Cardoso e Silva 6 Medeiros, Cláudia 7 Sibeck, D. G. 8 Kanekal, Shrikanth G. 9 Blake, J. B. 10 Kletzing, C. 11 Baker, D. |
Grupo | 1 DIHPA-CGCE-INPE-MCTI-GOV-BR 2 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR 3 DIHPA-CGCE-INPE-MCTI-GOV-BR 4 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR 5 DIHPA-CGCE-INPE-MCTI-GOV-BR 6 CORCR-CGIP-INPE-MCTI-GOV-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 NASA Goddard Space Flight Center 8 NASA Goddard Space Flight Center 9 The Aerospace Corporation 10 University of Iowa 11 University of Colorado |
Endereço de e-Mail do Autor | 1 ligia.alves01@gmail.com 2 grazybdias@hotmail.com 3 ligia.alves01@gmail.com 4 5 vitormoura21@gmail.com 6 claudia.inpe@gmail.com |
Nome do Evento | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA) |
Localização do Evento | Online |
Data | 22-26 mar. |
Histórico (UTC) | 2021-03-25 12:12:22 :: simone -> administrator :: 2022-04-03 23:14:49 :: administrator -> simone :: 2021 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Resumo | The key question on the Earths radiation belts trapped particles lies in the understanding of how solar wind drives the magnetospheric physical mechanisms changing the trapped particle populations. Corotating Interaction Regions (CIR) from Coronal Holes (CH) are predominant structures through the descending phase of the solar cycle. Some of the solar wind conditions related to CIRs are also recurrent in each rotation, so these structures may also cause a recurrent magnetospheric response to the solar wind coupling, including the inner magnetospheric parameters, in particular at the outer radiation belt dynamics. Throughout the descending phase of the solar cycle 24, we identified 46 CIRs in the period from 2016-2019. All the CIRs are isolated solar wind structures, i.e. complex solar wind structures are out of the scope of this paper. By following seven recurrences of CH 838, we identified recurrent magnetospheric auroral disturbances, besides inner magnetosphere seed population particle injection, and as a consequence, whistler-mode chorus waves are observed in a wide frequency range and in several L-shells and Magnetic Local Time. The unprecedented Van Allen Probes observation of very low frequency (VLF) waves show that for two subsequent orbits, whistler-mode chorus waves frequency bands alternates from one satellite passage to the other, being observed in several frequency ranges during the same solar wind event.. As a result, the relativistic outer radiation belt electron fluxes can be lost and enhance each time, as a function of the chorus waves power spectral density, thus the survey of outer radiation belt particle flux from several CIR events results that dropout, enhancement or no change may occur with the same likelihood (∼ 25%) each. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > How Does Relativistic... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > How Does Relativistic... |
Arranjo 3 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGIP > How Does Relativistic... |
Conteúdo da Pasta doc | não têm arquivos |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Grupo de Usuários | simone |
Visibilidade | shown |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3F2PBEE 8JMKD3MGPCW/46KTFK8 8JMKD3MGPCW/46KUES5 |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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