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1. Identity statement
Reference TypeConference Abstract (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3SB3SLB
Repositorysid.inpe.br/mtc-m21c/2018/12.03.15.15
Last Update2020:11.09.10.20.59 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2018/12.03.15.15.06
Metadata Last Update2020:11.09.10.20.59 (UTC) simone
Secondary KeyINPE--PRE/
Citation KeySousasantosKhSoAbMoSi:2018:ThPe
TitleA numerical study on the Equatorial Plasma Bubble seeded by the pre-reversal vertical drift: A three-dimensional perspective
Year2018
Access Date2024, May 09
Secondary TypePRE CI
Number of Files1
Size67 KiB
2. Context
Author1 Sousasantos, Jonas
2 Kherani, Esfhan Alam
3 Sobral, José Humberto Andrade
4 Abdu, Mangalathayil Ali
5 Moraes, Alison de Oliveira
6 Silva, André Luiz da
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHHA
4 8JMKD3MGP5W/3C9JHNK
Group1
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Tecnologico de Aeronáutica (ITA)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto de Aeronáutica e Espaço (IAE)
6 Instituto Tecnológico de Aeronáutica (ITA)
Author e-Mail Address1
2 esfhan.kherani@inpe.br
3
4 ma.abdu@inpe.br
Conference NameAGU Fall Meeting
Conference LocationWashington, D. C.
Date10-14 dec.
Book TitleAbstracts
History (UTC)2018-12-03 15:15:06 :: simone -> administrator ::
2019-01-14 17:06:39 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractDuring the last decades several seeding sources mechanisms were proposed to explain the generation of large scale depletions in the equatorial and low latitudes plasma know as Equatorial Plasma Bubble Structures. Numerical simulations have used direct density perturbations with couple of shapes, gravity waves, etc. In this work the pre-reversal mechanism is evaluated without the contribution of none of these external sources of perturbation. The variation of the vertical drift during its pre-reversal period in time and space was already suggested as a potential seeding source mechanism and this hypothesis was tested bidimensionally, however, the ambient conditions for a effective action of such seeding mechanism was found to be severe. The three-dimensional approach intents to evaluate a more realistic scenario, where the parallel conductivity could decrease substantially the action of the proposed mechanism. The results indicate that the mechanism is efficent in the instability seeding even in face of a more unfavorable scenario.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > A numerical study...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 03/12/2018 13:15 1.0 KiB 
4. Conditions of access and use
data URLhttp://mtc-m21c.sid.inpe.br/ibi/8JMKD3MGP3W34R/3SB3SLB
zipped data URLhttp://mtc-m21c.sid.inpe.br/zip/8JMKD3MGP3W34R/3SB3SLB
Languageen
Target Filesousasantos_numerical.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.54.26 2
sid.inpe.br/mtc-m21/2012/07.13.14.52.02 2
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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