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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/3PDMPR8
Repositorysid.inpe.br/mtc-m21b/2017/08.08.18.55
Last Update2017:08.08.18.55.05 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/08.08.18.55.05
Metadata Last Update2018:06.04.02.27.38 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeySilvaTakaWrasFigu:2017:CaIoPl
TitleCaracteristics of ionospheric plasma bubbles observed by tec maps in brazilian sector
Year2017
Access Date2024, May 09
Secondary TypePRE CI
Number of Files1
Size1030 KiB
2. Context
Author1 Silva, Diego Barros
2 Takahashi, Hisao
3 Wrasse, Cristiano Max
4 Figueiredo, Cosme Alexandre Oliveira Barros
Resume Identifier1
2 8JMKD3MGP5W/3C9JHCM
Group1 GES-CEA-SESPG-INPE-MCTIC-GOV-BR
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
4 GES-CEA-SESPG-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 diego.barros@inpe.br
2
3 cristiano.wrasse@inpe.br
4 cosme.figueiredo@inpe.br
Conference NameInternational Congress of the Brazilian Geophysical Sociey, 15
Conference LocationRio de Janeiro, RJ
Date31 jul. - 03 ago.
History (UTC)2017-08-08 18:55:32 :: simone -> administrator :: 2017
2018-06-04 02:27:38 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractUsing ionospheric TEC (Total Electron Content) maps provided by the Embrace Program/INPE (Brazilian Space Weather Study and Monitoring) it was possible to characterize the ionospheric plasma bubbles, the zonal drift velocity and the distance between consecutive bubbles observed in the Brazilian equatorial region from November 2012 to January 2016. The TEC maps were analyzed using the keogram technique. The data with more than 400 nights were analyzed with the presence of plasma bubbles between 18-03 HL (local time). The observed mean zonal drift velocities were between 65 and 125 m/s and the mean distances between consecutive plasma bubbles were between 640 and 900 km, these values being greater than previously observed. The results show that the ionospheric plasma bubbles present a significant latitudinal gradient in both zonal drift velocity and the distance between bubbles. In addition, the decrease of zonal drift velocities during a night was more clear to see in the region near the equatorial ionization anomaly.
AreaCEA
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34P/3PDMPR8
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34P/3PDMPR8
Target Filesilva_characteristics.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/bibdigital/2013/10.12.21.02 2
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url volume
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