| 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/3TKKMKL | |||
| Repositório | sid.inpe.br/mtc-m21c/2019/07.10.12.30 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21c/2019/07.10.12.30.03 | |||
| Última Atualização dos Metadados | 2020:01.06.11.42.16 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | CandidoSBCWKCLS:2019:HiStCo | |||
| Título | High-speed streams, Corotating Interaction Region, and HILDCAAs as important drivers of the ionospheric variability during low solar activity  | |||
| Ano | 2019 | |||
| Data de Acesso | 27 abr. 2024 | |||
| Tipo Secundário | PRE CI | |||
| 2. Contextualização | ||||
| Autor | 1 Candido, Cláudia Maria Nicoli 2 Shi, J. 3 Becker Guedes, Fábio 4 Correia, Emília 5 Wang, C. 6 Klausner, V. 7 Cecatto, José Roberto 8 Liu, Z. 9 Santos, S. | |||
| Identificador de Curriculo | 1 2 3 4 8JMKD3MGP5W/3C9JH2C 5 6 7 8JMKD3MGP5W/3C9JHJB | |||
| Grupo | 1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR 2 3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR 4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR 5 6 7 DIDAS-CGCEA-INPE-MCTIC-GOV-BR 8 9 DIDAE-CGCEA-INPE-MCTIC-GOV-BR | |||
| Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 National Science Space Center - NSSC, State Key Laboratory 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 National Science Space Center - NSSC, State Key Laboratory 6 Universidade do Vale do Paraíba (UNIVAP) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 ational Science Space Center - NSSC, China Brazil Jont Laboratory for Space Weather 9 Instituto Nacional de Pesquisas Espaciais (INPE) | |||
| Endereço de e-Mail do Autor | 1 claudia.candido@inpe.br 2 3 fabio.guedes@inpe.br 4 emilia.correia@inpe.br 5 6 7 jr.cecatto@inpe.br | |||
| Nome do Evento | IUGG General Assembly, 27 | |||
| Localização do Evento | Montréal, Canada | |||
| Data | 08-18 July | |||
| Histórico (UTC) | 2019-07-10 12:30:03 :: simone -> administrator :: 2019-07-14 22:45:16 :: administrator -> simone :: 2019 2019-12-06 18:53:36 :: simone -> administrator :: 2019 2020-01-06 11:42:16 :: administrator -> simone :: 2019 | |||
| 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 | Coronal holes are unipolar magnetic-field in the solar corona mostly observed at equatorial region during declining or minimum phase of the solar cycle. Their open magnetic field configuration allows the escape of particles and ions as high-speed solar wind streams. As they propagate in the interplanetary space, they form complex interactions regions which reach the geospace causing geomagnetic storms. Generally, a variety of effects are observed after the beginning of the geomagnetic storm, as it is important to understand the most important factors which impact the upper atmosphere and ionosphere. Combined events related to coronal holes and active regions in the Sun can also be observed. In this work, the ionospheric response at an equatorial region in the Brazilian sector to long duration recurrent coronal holes and their associated geomagnetic storms during the descending phase of the solar cycle 24 is investigated. For this purpose, we used instruments including GNSS receivers, ionosondes, and other ground-based systems. During the distinct Carrington, rotations are possible to observe a variety of ionospheric effects such as ionization decreases and increases, development of plasma bubbles and scintillation processes as a result of a combination of processes including prompt penetration of electric field, disturbance dynamo and the occurrence of high-intensity long duration auroral activity. This study may be useful for ionospheric modeling and Space Weather. | |||
| Área | CEA | |||
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > High-speed streams, Corotating... | |||
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > High-speed streams, Corotating... | |||
| 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 | ||||
| Grupo de Usuários | simone | |||
| Grupo de Leitores | administrator simone | |||
| Visibilidade | shown | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETL868 8JMKD3MGPCW/3ETR8EH | |||
| 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 language 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 | ||||