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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3K3B3LB
Repositóriosid.inpe.br/mtc-m21b/2015/08.11.12.42
Repositório de Metadadossid.inpe.br/mtc-m21b/2015/08.11.12.42.18
Última Atualização dos Metadados2018:06.04.02.55.37 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoAbdu:2015:PrWaSt
TítuloPrecursor wave structure, polarization electric field and vertical drift as drivers for equatorial plasma bubble/spread F development
Ano2015
Data de Acesso06 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
AutorAbdu, Mangalathayil Ali
Identificador de Curriculo8JMKD3MGP5W/3C9JHNK
GrupoDAE-CEA-INPE-MCTI-GOV-BR
AfiliaçãoInstituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autorma.abdu@inpe.br
Nome do EventoAnnual Meetings Asia Oceania Geosciences Society (AOGS)
Localização do EventoSingapore
Data2-7 Aug.
Histórico (UTC)2015-08-11 12:42:18 :: simone -> administrator ::
2018-06-04 02:55:37 :: administrator -> simone :: 2015
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoThe plasma bubble/spread F irregularities of the nighttime equatorial ionosphere typically develop in the post sunset hours, and often continue till sunrise. The irregularities develop from the R-T instability mechanism operating at the bottomside of an F layer in rapid rise under an enhanced evening prereversal zonal electric field (PRE). A precursor seed perturbation in electron density with polarization electric field, to be present at the steep density gradient region of the F layer bottomside, is an additional requirement, as per theoretical considerations and model studies. Recent results from both statistical as well as case studies bases have supported the presence of such perturbations in the form of wave structures, likely produced by upward propagating gravity waves. An important issue concerns the complementary/competing influences from the PRE and seed perturbation in the ESF development process. Of particular interest are the characteristics of the precursor wave structure in the hours preceding the post sunset ESF development, as diagnosed by different observational techniques. Analysis of the F layer heights at specific plasma frequencies as measured by Digisondes operated at equatorial and low latitude sites, including magnetic conjugate sites, in Brazil has revealed the characteristics of precursor wave structure in the form of gravity wave oscillations and their amplification in the afternoon hours leading to post sunset ESF development. In this talk we will present and discuss recent results on the characteristics of the precursor wave structure as seen by different techniques, and in particular the observations by Digisondes showing evidence on its sustenance and amplification in the afternoon hours, supported by model results, and the relationship to the PRE and post sunset ESF development.
ÁreaCEA
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4. Condições de acesso e uso
Grupo de Usuáriossimone
Visibilidadeshown
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhourlib.net/www/2011/03.29.20.55
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
Lista de Itens Citando 1
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
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