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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/3D72L32
Repositorysid.inpe.br/mtc-m19/2012/12.10.18.27
Last Update2020:11.25.13.22.55 (UTC) marcelo.pazos@inpe.br
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.10.18.27.03
Metadata Last Update2020:11.25.13.22.56 (UTC) marcelo.pazos@inpe.br
Secondary KeyINPE--PRE/
Labelself-archiving-INPE-MCTIC-GOV-BR
Citation KeyResendeNarBatMorGui:2012:StDiBl
TitleA study of different blanketing Es layers during the solar cycle 23
Year2012
Access Date2024, May 19
Secondary TypePRE CI
Number of Files1
Size35 KiB
2. Context
Author1 Resende, Laysa Cristina Araújo
2 De Nardini, Clezio Marcos
3 Batista, Inez Staciarini
4 Moro, Juliano
5 Guizelli, Lais Maria
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHDA
Group1
2
3 DAE-CEA-INPE-MCTI-GOV-BR
Affiliation1
2
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3 inez@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)2013-02-27 13:24:36 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:24 :: 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
Version Typepublisher
AbstractWe investigate the behavior of blanketing frequency (fbEs) measured by a digital ionosonde over São Luís, Brazil (2.33°S, 44.2°W, dip: -4.5°), associated with different types of Es, according to the magnetic disturbance level and, in relation to the phase of strong magnetic storms that occured during the solar cycle 23. Our preliminary results showed that there are expressive changes in the fbEs characterized by occurrence of peaks that exceeds the ambient background values, mainly during the recovery phase of strong magnetic storms. These peaks are associated to the presence of blanketing Es types, which are not the common Es at the dip equator but replaced the Esq, a non-blanketing layer observed in ionograms due the plasma irregularities in the equatorial electrojet electric field. Therefore, we suppose the wind shear mechanism is taking place at latitudes close to the dip equator, where it is not supposed to operate efficiently. The results are discussed in terms of the statistics of the abnormal enhancement taking into account the magnetic disturbance level and phase of the magnetic storm, when applicable.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > A study of...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3D72L32
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3D72L32
Target Fileresende_study.pdf
User Groupmarcelo.pazos@inpe.br
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETL868
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 tertiarymark type url volume
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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