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1. Identity statement
Reference TypeConference Abstract (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D6FDFP
Repositorysid.inpe.br/mtc-m19/2012/12.07.12.35
Last Update2021:03.01.15.11.59 (UTC) marcelo.pazos@inpe.br
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.07.12.35.19
Metadata Last Update2021:03.01.15.12.00 (UTC) marcelo.pazos@inpe.br
Secondary KeyINPE--PRE/
Labelself-archiving-INPE-MCTIC-GOV-BR
Citation KeyElyBatiCarr:2012:VeExDr
TitleVertical ExB drift during pre-reversal peak hours at magnetically conjugate stations in Brazil (COPEX Campaign) using digisonde data
Year2012
Access Date2024, May 19
Secondary TypePRE CI
Number of Files1
Size35 KiB
2. Context
Author1 Ely, Cláudia Vogel
2 Batista, Inez Staciarini
3 Carrasco, Alexander José
Resume Identifier1
2 8JMKD3MGP5W/3C9JHDA
Group1 DAE-CEA-INPE-MCTI-GOV-BR
2 DAE-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 claudia.ely@dae.inpe.br
e-Mail Addressmarcelo.pazos@inpe.br
Conference NameInternational Symposium on Equatorial Aeronomy, 13 (ISEA).
Conference LocationParacas, Peru
Date12 a 17/03/2012
Book TitleAbstracts
Tertiary TypePoster
History (UTC)2013-02-28 11:31:29 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:16 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe time variation of the F layer height at specific frequencies (dh(f)/dt) can be used to estimate the vertical plasma velocity of the F layer. This apparent velocity has contributions from the electromagnetic ExB drift, from the meridional neutral wind and from the height variations due to recombination, but close to the magnetic equator and near sunset, when the F layer is high enough for the recombination process to be considered negligible, the electromagnetic ExB becomes the most important component. This paper will present the temporal variations of the vertical drift approximated with the above technique and also the vertical plasma velocity derived using a new technique based on the numerical solution of the continuity equation, both obtained for the quietest days from the COPEX campaign (October to December of 2002, high solar activity) near sunset hours. We will compare the vertical ExB drift simultaneously in two magnetically conjugated stations and at a magnetic equator station, and analyze the differences and their possible causes in terms of meridional winds.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Vertical ExB drift...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 07/12/2012 10:35 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3D6FDFP
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3D6FDFP
Target Fileely_vertical.pdf
User Groupmarcelo.pazos@inpe.br
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho Vinculado à Tese/Dissertação
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor format isbn issn keywords language lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject type url versiontype volume
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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