| 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/47N6AUP | |||
| Repositório | sid.inpe.br/mtc-m21d/2022/09.30.10.47 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21d/2022/09.30.10.47.50 | |||
| Última Atualização dos Metadados | 2023:01.03.16.46.18 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | AdebayoPime:2022:CoInRe | |||
| Título | Comprehensive Investigation of the Relationship Between Equatorial Plasma Bubbles and Plasma Blobs Using Optical and Radio Techniques and Multi-Satellite Data  | |||
| Ano | 2022 | |||
| Data de Acesso | 12 maio 2024 | |||
| Tipo Secundário | PRE CI | |||
| 2. Contextualização | ||||
| Autor | 1 Adebayo, Oluwasegun Micheal 2 Pimenta, Alexandre Alvares | |||
| Identificador de Curriculo | 1 2 8JMKD3MGP5W/3C9JGGL | |||
| Grupo | 1 DICEP-CGCE-INPE-MCTI-GOV-BR 2 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) | |||
| Endereço de e-Mail do Autor | 1 adebayooluwasegun37@gmail.com 2 alvarespimenta@hotmail.com | |||
| Nome do Evento | International Symposium on Equatorial Aeronomy, 16 | |||
| Localização do Evento | Kyoto, Japan | |||
| Data | 12-16 Sept. 2022 | |||
| Histórico (UTC) | 2022-09-30 10:47:50 :: simone -> administrator :: 2023-01-03 16:46:18 :: administrator -> simone :: 2022 | |||
| 3. Conteúdo e estrutura | ||||
| É a matriz ou uma cópia? | é a matriz | |||
| Estágio do Conteúdo | concluido | |||
| Transferível | 1 | |||
| Tipo do Conteúdo | External Contribution | |||
| Palavras-Chave | plasma bubbles plasma blobs occurrence patterns all-sky imagers multi-satellite | |||
| Resumo | Plasma bubbles and plasma blobs are night-time consequences of F-region plasma instability. Irregularities behaviour of plasma in the ionosphere poses adverse effects on our technologically-inclined daily activities. In the full capacity of these phenomena, we could lose communications with satellite, aircraft to mention few. Hence, it is imperative for us to investigate these phenomena continuously. The relationships between the two phenomena have been a subject of research recently and debates still persist regarding whether both phenomena are independent or causally related. Earlier works were more or less of case studies while we present detailed occurrence characteristics of blobs and bubbles during high solar activity (HSA) and low solar activity (LSA) for the period of two years (one year for each solar activity). OI 630.0 nm emission images (about 3000 in total) from two similar all-sky imaging systems, digisonde and SWARM electron density, Ne, and electron temperature, Te, data have been used to investigate the relationship between plasma bubbles and plasma blobs. Monthly, seasonal, and nocturnal variations of bubbles and blobs are present in this work. During HSA, approximately 95% of plasma blobs observed were associated with plasma bubbles whereas every single blob observed during LSA were associated with bubbles (100%). However, not all the bubbles observed were associated with blobs. In other words, bubbles without blobs cases were observed. Correlation and regression analyses of the two phenomena revealed interesting causal relationship between bubbles and blobs. Approximated average visibility time of plasma blobs, based on its time of appearance and disappearance from the field of view, during HSA and LSA were 1.08 hr (approx. 65 mins) and 0.57 hr (approx. 34 mins), respectively. Whereas the average visibility time of plasma bubbles during HSA and LSA were 4.01 hr and 2.19 hr, respectively. Plasma blobs occurrence frequency had its maximum at around midnight hours whereas plasma bubble has its occurrence maximum frequency at around post-sunset hours. From these concise results and the ones obtained from the literature, we have been able to propose two distinct mechanisms for the development of plasma blobs: (1) plasma blobs associated with plasma bubbles; and (2) plasma blobs not associated with plasma bubbles. | |||
| Área | CEA | |||
| Arranjo | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Comprehensive Investigation of... | |||
| Conteúdo da Pasta doc | não têm arquivos | |||
| Conteúdo da Pasta source | não têm arquivos | |||
| Conteúdo da Pasta agreement |
| |||
| 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/46KTFK8 | |||
| Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notas | ||||
| Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup 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 | ||||