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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3RFFC3P
Repositorysid.inpe.br/mtc-m21c/2018/07.17.18.35
Metadata Repositorysid.inpe.br/mtc-m21c/2018/07.17.18.35.14
Metadata Last Update2022:03.18.22.11.20 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyBarrosSilvaTakWraFigCar:2018:ChEqPl
TitleCharacteristics of equatorial plasma bubbles observed by tec map over south america and numerical simulation of its development
Year2018
Access Date2024, May 08
Secondary TypePRE CI
2. Context
Author1 Barros Silva, Diego
2 Takahashi, Hisao
3 Wrasse, Cristiano Max
4 Figueiredo, Cosme Alexandre Oliveira Barros
5 Carrasco, Alexander J.
Resume Identifier1
2 8JMKD3MGP5W/3C9JHCM
Group1 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
2
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
4 GESAST-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)
5 Universidad de Los Andes
Author e-Mail Address1 diego.barros@inpe.br
2 hisao.takahashi@inpe.br
3 cristiano.wrasse@inpe.br
4 cosme.figueiredo@inpe.br
5 carrasco@ula.ve
Conference NameCospar Scientific Assembly, 42
Conference LocationPasadena, California
Date14-22 July
History (UTC)2018-07-17 18:35:50 :: simone -> administrator :: 2018
2018-07-19 05:41:39 :: administrator -> simone :: 2018
2018-08-08 11:44:16 :: simone -> administrator :: 2018
2022-03-18 22:11:20 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
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Content TypeExternal Contribution
AbstractGround-based network of GNSS receivers have been used to monitor Equatorial Plasma Bubbles (EPBs) by mapping the Total Electron Content (TEC map). Large coverage of the TEC map allowed us to monitor several EPBs simultaneously and get characteristics of the dynamics, extension and longitudinal distributions of the EPBs from the onset time until their disappearance. These characteristics were obtained by using TEC map analysis and keogram technique by using the data obtained during the period between November/2012 and January/2016. The zonal drift velocities of the EPBs showed a clear latitudinal gradient varying from 123 m/s at the equator to 65 m/s for 35°S of latitude. Consequently, observed EPBs are inclined against the geomagnetic field lines. Both zonal drift velocity and the inclination of the EPBs were compared with the thermospheric neutral wind, which showed a good agreement. Moreover, large coverage of TEC maps permit to study periodic EPBs with a wide longitudinal distance. This averaged values observed for the inter-bubbles distances also presented a clear latitudinal gradient varying from 920 km at the equator to 640 km at 30°S. On several occasions, the distances reached more than 2000 km. Inter-bubbles distances greater than 1000 km have not been reported in literature. Numerical model calculations, using different latitudinal gradients in zonal wind, showed a good agreement with the latitudinal gradient in the EPBs zonal drift observed by TEC map. Comparison of the observational results with the theoretical model calculations confirms that the EPB inclination against the geomagnetic field lines and the latitudinal gradient of inter-bubbles distances were originated due to a latitudinal gradient in the.
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User Groupsimone
Reader Groupadministrator
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Visibilityshown
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Mirror Repositoryurlib.net/www/2017/11.22.19.04.03
Next Higher Units8JMKD3MGPCW/3ETL868
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Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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