| 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/44CP24P | |||
| Repositório | sid.inpe.br/mtc-m21c/2021/03.23.12.17 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21c/2021/03.23.12.17.42 | |||
| Última Atualização dos Metadados | 2022:04.03.19.25.05 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | SilvaSRABSVWSJMDZL:2021:EnPaDy | |||
| Título | Energetic particle dynamic on the radiation belts and the generation of the sporadic E- layer (Esa) on the SHMA  | |||
| Ano | 2021 | |||
| Data de Acesso | 11 maio 2024 | |||
| Tipo Secundário | PRE CN | |||
| 2. Contextualização | ||||
| Autor | 1 Silva, L. A. 2 Shi, J. 3 Resende, Laysa Cristina Araújo 4 Alves, Livia Ribeiro 5 Batista, Inez Staciarini 6 Sibeck, D. 7 Vieira, Luis Eduardo Antunes 8 Wang, C. 9 Souza, Vitor Moura Cardoso e Silva 10 Jauer, P. R. 11 Marchezi, José Paulo 12 Denardini, Clezio Marcos 13 Zhang, S. Y. 14 Liu, Z. | |||
| Identificador de Curriculo | 1 2 3 4 5 8JMKD3MGP5W/3C9JHDA | |||
| Grupo | 1 2 3 DICEP-CGCE-INPE-MCTI-GOV-BR 4 DIHPA-CGCE-INPE-MCTI-GOV-BR 5 DIHPA-CGCE-INPE-MCTI-GOV-BR 6 7 DIHPA-CGCE-INPE-MCTI-GOV-BR 8 9 DIHPA-CGCE-INPE-MCTI-GOV-BR 10 11 12 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 State Key Laboratory of Space Weather 2 State Key Laboratory of Space Weather 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 NASA Goddard Space Flight Center 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 State Key Laboratory of Space Weather 9 Instituto Nacional de Pesquisas Espaciais (INPE) 10 State Key Laboratory of Space Weather 11 jose.marchezi@inpe.br 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Chinese Academy of Sciences 14 State Key Laboratory of Space Weather | |||
| Endereço de e-Mail do Autor | 1 2 3 laysa.resende@gmail.com 4 livia.alves@inpe.br 5 inez.batista@inpe.br 6 7 luis.vieira71@googlemail.com 8 9 vitormoura21@gmail.com 10 11 12 clezio.denardin@inpe.br | |||
| Nome do Evento | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA) | |||
| Localização do Evento | Online | |||
| Data | 22-26 mar. | |||
| Histórico (UTC) | 2021-03-23 12:17:42 :: simone -> administrator :: 2021-06-22 19:11:15 :: administrator -> simone :: 2021 2021-06-22 20:59:50 :: simone -> administrator :: 2021 2022-04-03 19:25:05 :: administrator -> simone :: 2021 | |||
| 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 energetic particle population in the radiation belts can be affected through the coupling between the solar wind structures and the Earths magnetosphere. When such particles precipitate into the upper atmosphere they may also affect both the ionosphere and the neutral atmosphere, especially at high-latitudes and the Southern Hemisphere Magnetic Anomaly (SHMA). Presently, the impact of the energetic particle precipitation into the highlatitude ionosphere is well understood. On the other hand, the direct impact into the SHMA ionosphere is still lacking in more information. Therefore, a case study (May 28, 2017) is selected during the strong geomagnetic-storm (Dst: -125 nT) associated with an Interplanetary Coronal Mass Ejection. The Van Allen Probes recorded a significant reduction on the radiation belts electron fluxes concomitant with a shock detected by ACE-satellite in the Interplanetary Medium. Particles in a wide range of energy levels were lost to the atmosphere. POES satellite data and FengYun series spacecraft 3C confirm a strong increase of the energetic particle flux in the SHMA region during this storm. Data from a digisonde installed near the center of the SHMA (29.68◦S, 53.81◦W) show the type sporadic E-layer (Esa), unusual in low-latitudes, during several hours. The increase of charged particles in this region can be related to the generation of the Esa layers, which occurrence is associated with particle precipitation. We conclude that the radiation belt dynamics, as well as the particle precipitation on the SHMA region during this storm, are the main components responsible for the generation of the Esa layers over the Brazilian region. | |||
| Área | CEA | |||
| Arranjo | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Energetic particle dynamic... | |||
| 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 | |||
| Grupo de Leitores | administrator simone | |||
| Visibilidade | shown | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/46KTFK8 | |||
| Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 | |||
| 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 readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||