| 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/3SEQ8S5 | |||
| Repositório | sid.inpe.br/mtc-m21c/2018/12.26.17.20 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21c/2018/12.26.17.20.07 | |||
| Última Atualização dos Metadados | 2022:03.18.22.11.26 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | JauerSPWAADVLECDSDMMSBS:2018:CoInRe | |||
| Título | A global magnetohydrodynamic simulation study of ultra-low frequency waves activity in the inner magnetosphere: corotating interaction region + alfvenic fluctuations  | |||
| Ano | 2018 | |||
| Data de Acesso | 11 maio 2024 | |||
| Tipo Secundário | PRE CN | |||
| 2. Contextualização | ||||
| Autor | 1 Jauer, Paulo Ricardo 2 Souza, Vitor Moura Cardoso e Silva 3 Pádua, Marcelo Banik de 4 Wang, C. 5 Alves, Maria Virginia 6 Alves, Livia Ribeiro 7 Da Silva, L. S. 8 Vieira, Luís Eduardo Antunes 9 Lopez, R. E. 10 Echer, Ezequiel 11 Costa, Joaquim Eduardo Rezende 12 Denardin, Clezio Marcos 13 Silva, Marlos Rockenbach da 14 Deggeroni, Vinicius 15 Medeiros, Cláudia 16 Marchezi, José Paulo 17 Silva, G. 18 Barbosa, Marcos Vinícius Grala 19 Schmitz, Roberta Gonçalves | |||
| Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JHNR 4 5 8JMKD3MGP5W/3C9JHRS 6 7 8 9 10 8JMKD3MGP5W/3C9JH3D 11 8JMKD3MGP5W/3C9JHF8 | |||
| Grupo | 1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 4 5 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 6 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 7 8 DIDAS-CGCEA-INPE-MCTIC-GOV-BR 9 10 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 11 DIDAS-CGCEA-INPE-MCTIC-GOV-BR 12 CGCEA-CGCEA-INPE-MCTIC-GOV-BR 13 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 14 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 15 COCRC-COCRC-INPE-MCTIC-GOV-BR 16 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 17 18 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 19 GESAST-CEA-SESPG-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 State Key Laboratory of Space Weather (NSSC/CAS) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 University of Texas at Arlington 10 Instituto Nacional de Pesquisas Espaciais (INPE) 11 Instituto Nacional de Pesquisas Espaciais (INPE) 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Instituto Nacional de Pesquisas Espaciais (INPE) 14 Instituto Nacional de Pesquisas Espaciais (INPE) 15 Instituto Nacional de Pesquisas Espaciais (INPE) 16 Instituto Nacional de Pesquisas Espaciais (INPE) 17 Instituto Nacional de Pesquisas Espaciais (INPE) 18 Instituto Nacional de Pesquisas Espaciais (INPE) 19 Instituto Nacional de Pesquisas Espaciais (INPE) | |||
| Endereço de e-Mail do Autor | 1 pauloricardojauer@gmail.com 2 vitor.souza@inpe.br 3 marcelo.padua@inpe.br 4 5 mv.alves@inpe.br 6 livia.alves@inpe.br 7 8 luiz.vieira@inpe.br 9 10 ezequiel.echer@inpe.br 11 joaquim.costa@inpe.br 12 clezio.denardin@inpe.br 13 marlos.silva@inpe.br 14 vinicius.deggeroni@inpe.br 15 claudia.medeiros@inpe.br 16 jose.marchezi@inpe.br 17 18 marcos.barbosa@inpe.br 19 roberta.schmitz@inpe.br | |||
| Nome do Evento | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 7 (SBGEA) | |||
| Localização do Evento | Santa Maria, RS | |||
| Data | 05-09 nov | |||
| Histórico (UTC) | 2018-12-26 17:20:07 :: simone -> administrator :: 2019-01-04 16:57:17 :: administrator -> simone :: 2018 2019-01-07 13:09:10 :: simone -> administrator :: 2018 2022-03-18 22:11:26 :: 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 | |||
| Tipo de Versão | publisher | |||
| Resumo | The interaction between the disturbed solar wind and the geomagnetic field gives rise to different physical processes that can significantly affect technological systems as well as human life. The goal of this work is to investigate the role of a complex solar structure, i.e., a corotating interaction region (CIR) followed by solar winds magnetic field Alfvénic fluctuations, in the generation of disturbances in the inner magnetosphere in terms of the power spectral density (PSD) of the ultra low frequency waves (ULF) in the nightside, equatorial region. There are several studies that show the correlation between fluctuations of solar winds magnetic field and plasma parameters characteristic of CIRs and Alfvénic fluctuations and the corresponding generation of ULF waves in the internal magnetosphere. However, some issues remain, namely, during such a complex event it is not straightforward to decisively say which solar wind parameters or which combinations thereof are most effective in causing disturbances in the inner magnetosphere, or how each part of the complex interplanetary structure influences the most the temporal evolution of the magnetosphere. Using global magnetohydrodynamical (MHD) simulations we perform a study which try to address some of these questions. Firstly, we use the magnetic field and plasma parameters of a real, complex CIR+Alfvénic fluctuations event as input to the SWMF/BATS-R-US code and then calculate from the model outputs the PSD of ULF waves in the aforementioned region. Then, we separate the complex event into its constituent parts by building synthetic magnetic field and plasma profiles based on the physical parameters that characterize each of these parts. The MHD code is then fed with each new synthetic profile to provide ULF PSDs that are compared with those from the simulation with real solar wind inputs. This numerical experiment will help us to understand which solar wind parameters contribute the most for the ULF waves activity in the nightside magnetosphere, as far as MHD simulations are concerned, and which combination of these synthetic parameters can reproduce the results obtained when running the MHD code with input data from the actual event. This work might also provide important information for future forecasting studies of ULF wave activity in the Earths magnetosphere whenever the geospace is under the influence of recurrent events as the one analyzed here. | |||
| Área | CEA | |||
| 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 | pt | |||
| Grupo de Usuários | simone | |||
| Grupo de Leitores | administrator simone | |||
| Visibilidade | shown | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETR8EH 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EU2FR5 8JMKD3MGPCW/3F2PBEE 8JMKD3MGPCW/3F3PAJE | |||
| 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 volume | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||