| 1. Identificação | ||||
| Tipo de Referência | Artigo em Evento (Conference Proceedings) | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identificador | 8JMKD3MGP3W34T/4AC7QQB | |||
| Repositório | sid.inpe.br/mtc-m21d/2023/12.11.12.15 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21d/2023/12.11.12.15.08 | |||
| Última Atualização dos Metadados | 2024:01.02.17.16.56 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | AlvesSSSMJFDS:2023:OuRaBe | |||
| Título | Outer radiation belt electron flux response to enhanced solar wind speed daily average  | |||
| Ano | 2023 | |||
| Data de Acesso | 10 maio 2024 | |||
| Tipo Secundário | PRE CI | |||
| 2. Contextualização | ||||
| Autor | 1 Alves, Livia Ribeiro 2 Silva, Ligia Alves da 3 Silva, Graziela Belmira Dias da 4 Schaefer, Daiene M. 5 Marchezi, José Paulo 6 Jauer, Paulo Ricardo 7 Ferreira, Karen Júlia Coldebella 8 Deggeroni, Vinícius 9 Sibeck, David G. | |||
| Grupo | 1 DIHPA-CGCE-INPE-MCTI-GOV-BR 2 DIHPA-CGCE-INPE-MCTI-GOV-BR 3 DICEP-CGCE-INPE-MCTI-GOV-BR 4 5 6 DICEP-CGCE-INPE-MCTI-GOV-BR 7 GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR 8 GESAST-CEA-DIPGR-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 Universidade Tecnológica Federal do Paraná (UTFPR) 5 University of New Hampshire Main Campus 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 NASA/GSFC | |||
| Endereço de e-Mail do Autor | 1 livia.alves@inpe.br 2 ligia.silva@inpe.br 3 graziela.silva@inpe.br 4 5 6 paulo.jauer@inpe.br 7 karen.ferreira@inpe.br 8 vinicius.deggeroni@inpe.br | |||
| Nome do Evento | AGU FAll Meeting | |||
| Localização do Evento | San Francisco, CA | |||
| Data | 11-15 Dec. 2023 | |||
| Editora (Publisher) | AGU | |||
| Título do Livro | Proceedings | |||
| Histórico (UTC) | 2023-12-11 12:15:08 :: simone -> administrator :: 2024-01-02 17:16:56 :: administrator -> simone :: 2023 | |||
| 3. Conteúdo e estrutura | ||||
| É a matriz ou uma cópia? | é a matriz | |||
| Estágio do Conteúdo | concluido | |||
| Transferível | 1 | |||
| Tipo do Conteúdo | External Contribution | |||
| Tipo de Versão | publisher | |||
| Resumo | The relationship between relativistic electron fluxes in the radiation belts and the solar wind speed has been investigated since 1979 to determine how the outer radiation belt responds to increases in the solar wind speed. Since then, several papers have addressed electrons at geosynchronous orbit, and theorists have explained how increases in the solar wind speed can drive the Earth's magnetosphere. Among these advances, an important point is the distributions of outer radiation belt electron fluxes as a function of solar wind speed, as well as increases in magnetospheric wave activity during these periods. This work determines the upper limit of the outer radiation belt electron fluxes as a function of solar wind speed, in addition to the magnetospheric wave activity that contributes to enhanced relativistic electron fluxes. We analyze the daily average of the solar wind speed and outer radiation belt electron fluxes with energies of 1.8 MeV, 2.1 MeV, 2.6 MeV, and 3.4 MeV at several L-shells (4, 4.5, and 5). Also, we consider the daily average of the ULF wave power in the Pc5 frequency range (2-5 mHz) which is often invoked to account for inward diffusion. Data sets are provided by Van Allen Probes (2013-2018) and ACE satellite. Our results show that the outer radiation belt electron flux reaches more than 2.5x106 cm2 s-1 sr-1 MeV-1 when daily averages of the solar wind speed surpass 500 km/s. Flux levels can remain enhanced for a long periods, leading to several days of enhanced fluxes even for low solar wind speeds. Generally, we observe that solar wind speed varies as the solar cycle progress. Eventually, solar wind events can reach fast speeds (on average) and, thus, the change in the electron flux distribution in the outer radiation belt is more often observed. Our results aim to contribute to the understanding of the physical processes involved in the outer radiation belt electron flux enhancements during fast solar wind streams. | |||
| Área | CEA | |||
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Outer radiation belt... | |||
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Outer radiation belt... | |||
| 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 | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3F2PBEE 8JMKD3MGPCW/46KTFK8 | |||
| Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notas | ||||
| Campos Vazios | archivingpolicy archivist 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 publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url volume | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||