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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/43MN648
Repositorysid.inpe.br/mtc-m21c/2020/12.02.14.25
Last Update2020:12.02.14.25.33 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2020/12.02.14.25.33
Metadata Last Update2022:01.04.01.35.41 (UTC) administrator
DOI10.1029/2020JA028609
ISSN2169-9402
Citation KeyCarrascoPimWraBatTak:2020:WhEqPl
TitleWhy Do Equatorial Plasma Bubbles Bifurcate?
Year2020
MonthNov.
Access Date2024, May 09
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2366 KiB
2. Context
Author1 Carrasco, Alexander José
2 Pimenta, Alexandre Alvares
3 Wrasse, Cristiano Max
4 Batista, Inez Staciarini
5 Takahashi, Hisao
Resume Identifier1
2 8JMKD3MGP5W/3C9JGGL
3
4 8JMKD3MGP5W/3C9JHDA
5 8JMKD3MGP5W/3C9JHCM
ORCID1 0000-0002-6182-8077
Group1
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
5 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 University of Los Andes
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 layerf2@gmail.com
2 alexandre.pimenta@inpe.br
3 christiano.wrasse@inpe.br
4 inez.batista@inpe.br
5 hisao.takahashi@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume125
Number11
Pagese2020JA028609
History (UTC)2020-12-02 14:25:33 :: simone -> administrator ::
2020-12-02 14:25:34 :: administrator -> simone :: 2020
2020-12-02 14:26:39 :: simone -> administrator :: 2020
2020-12-03 22:57:30 :: administrator -> simone :: 2020
2020-12-14 14:01:23 :: simone -> administrator :: 2020
2022-01-04 01:35:41 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractIonospheric plasma bubble observations using all-sky airglow imagers in the OI 630-nm emission show bifurcations with complex patterns. Bifurcation is the division of one channel of the plasma bubble into two that grow vertically in the magnetic equator. Several theories have been suggested to explain the bifurcation mechanism. In this work we use a plasma bubble simulation code to examine these theories. The model used shows that the height where the bifurcation occurs is conditioned by the polarization electric fields inside the bubble. The numerical simulation produced plasma bubbles with complex ramifications which agree with the observations taken at São João do Cariri (7.4°S, 36.5°W).
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Why Do Equatorial...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 02/12/2020 11:25 1.0 KiB 
4. Conditions of access and use
data URLhttp://mtc-m21c.sid.inpe.br/ibi/8JMKD3MGP3W34R/43MN648
zipped data URLhttp://mtc-m21c.sid.inpe.br/zip/8JMKD3MGP3W34R/43MN648
Languageen
Target Filecarrasco_why.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/bibdigital/2013/09.29.20.43 2
sid.inpe.br/mtc-m21/2012/07.13.14.50.14 2
sid.inpe.br/mtc-m21/2012/07.13.14.49.58 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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