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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3K3B3LB
Repositorysid.inpe.br/mtc-m21b/2015/08.11.12.42
Metadata Repositorysid.inpe.br/mtc-m21b/2015/08.11.12.42.18
Metadata Last Update2018:06.04.02.55.37 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyAbdu:2015:PrWaSt
TitlePrecursor wave structure, polarization electric field and vertical drift as drivers for equatorial plasma bubble/spread F development
Year2015
Access Date2024, May 20
Secondary TypePRE CI
2. Context
AuthorAbdu, Mangalathayil Ali
Resume Identifier8JMKD3MGP5W/3C9JHNK
GroupDAE-CEA-INPE-MCTI-GOV-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Addressma.abdu@inpe.br
Conference NameAnnual Meetings Asia Oceania Geosciences Society (AOGS)
Conference LocationSingapore
Date2-7 Aug.
History (UTC)2015-08-11 12:42:18 :: simone -> administrator ::
2018-06-04 02:55:37 :: administrator -> simone :: 2015
3. Content and structure
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AbstractThe 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.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Precursor wave structure,...
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5. Allied materials
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item List 1
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
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