| 1. Identificação | ||||
| Tipo de Referência | Slides (Audiovisual Material) | |||
| Site | mtc-m21c.sid.inpe.br | |||
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identificador | 8JMKD3MGP3W34R/43UNHQ2 | |||
| Repositório | sid.inpe.br/mtc-m21c/2021/01.14.18.09 | |||
| Última Atualização | 2021:01.14.18.09.10 (UTC) administrator | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21c/2021/01.14.18.09.10 | |||
| Última Atualização dos Metadados | 2021:09.16.03.39.41 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | MarcheziAlSiSiKaBa:2018:InReEl | |||
| Título | Increase in relativistic electron flux density during an complex interplanetary structure on 09 February 2014  | |||
| Título Curto | Slides | |||
| Formato | On-line | |||
| Ano | 2018 | |||
| Data de Acesso | 18 maio 2024 | |||
| Tipo Secundário | PRE CI | |||
| Número de Arquivos | 1 | |||
| Tamanho | 1765 KiB | |||
| 2. Contextualização | ||||
| Autor | 1 Marchezi, José Paulo 2 Alves, Livia Ribeiro 3 Silva, Ligia Alves da 4 Sibeck, David G. 5 Kanekal, Shrikanth G. 6 Baker, Daniel N. | |||
| Grupo | 1 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 3 DIDGE-CGCEA-INPE-MCTIC-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 NASA Goddard Space Flight Center 5 NASA Goddard Space Flight Center 6 University of Colorado | |||
| Endereço de e-Mail do Autor | 1 jose.marchezi@inpe.br 2 livia.alves@inpe.br 3 ligia.silva@inpe.br | |||
| Nome do Evento | AGU Fall Meeting | |||
| Localização do Evento | Washington, D. C. | |||
| Data | 10-14 dec. | |||
| Editora (Publisher) | Instituto Nacional de Pesquisas Espaciais | |||
| Cidade da Editora | São José dos Campos | |||
| Histórico (UTC) | 2021-01-14 18:09:10 :: simone -> administrator :: 2021-09-16 03:39:41 :: administrator -> simone :: 2018 | |||
| 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 particles trapped in the Earth's magnetic field perform three typical movements: gyromotion around the magnetic field line, bouncing along the magnetic field line and drifting across the magnetic field lines. Each movement has a characteristic time and constant of motion called the adiabatic invariant. The solar wind perturbations can interact with the Earth's magnetosphere and generate waves that have frequencies resonant with the characteristic frequencies of the adiabatic motion. With frequencies in the same range as those of the particle drift, ultra-low frequency (ULF) waves are known to cause significant changes in the energetic particle flux in the outer radiation belts. On 09 February 2014, the ACE satellite detected solar wind plasma and Interplanetary Magnetic Field (IMF) perturbations related to an Interplanetary Mass Ejection (ICME) followed by a High Speed Solar Wind Stream (HSS) event. In this work, we analyze the recovery of relativistic outer radiation belt electron flux after the interaction of a complex interplanetary structure with the Earths magnetosphere. We are interested in the HSS period, around 18:00 UT, when the outer radiation belt electrons flux density exhibited a gradual increase only a few hours after the interplanetary structure arrived. The electron flux density data where obtained by the Relativistic Electron Proton Telescope (REPT) instrument, onboard of the Van Allen Probes. For that period, the Probes where located at MLT ~ 15 and L ~ 5. The north-south solar wind magnetic field is characterized by a predominantly negative Bz and Alfvénic fluctuations. The main focus here is to evaluate the role of each ULF wave frequency range, corresponding to Pc3, Pc4 and Pc5, in accelerating outer radiation belt electrons. Observations show an increase in the ULF wave power spectrum density for the electric and magnetic fields at the Van Allen Probes corresponding to an enhancement of the electron flux density with energies from 1.80 up to 3.40 MeV. This may indicate that ULF waves play a more important role on the acceleration process for this complex event. | |||
| Área | CEA | |||
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Slides | |||
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Slides | |||
| Arranjo 3 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Increase in relativistic... > Slides | |||
| Arranjo 4 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Increase in relativistic... > Slides | |||
| Conteúdo da Pasta doc | acessar | |||
| Conteúdo da Pasta source | não têm arquivos | |||
| Conteúdo da Pasta agreement |
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| 4. Condições de acesso e uso | ||||
| URL dos dados | http://urlib.net/ibi/8JMKD3MGP3W34R/43UNHQ2 | |||
| URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP3W34R/43UNHQ2 | |||
| Idioma | en | |||
| Arquivo Alvo | marchezi_increase_poster.pdf | |||
| Grupo de Usuários | simone | |||
| Visibilidade | shown | |||
| Permissão de Leitura | allow from all | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3F2PBEE 8JMKD3MGP3W34R/3SB3GME | |||
| Lista de Itens Citando | sid.inpe.br/bibdigital/2013/10.12.21.02 3 | |||
| Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 | |||
| 6. Notas | ||||
| Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress isbn issn keywords label lineage mark mirrorrepository nextedition notes numberofslides orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session sponsor subject tertiarymark tertiarytype type url versiontype volume | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||