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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4878ESP
Repositorysid.inpe.br/mtc-m21d/2022/12.13.17.59
Metadata Repositorysid.inpe.br/mtc-m21d/2022/12.13.17.59.53
Metadata Last Update2023:01.03.16.46.27 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeySilvaTakWraFigCar:2022:AsDeEq
TitleAsymmetric Development of Equatorial Plasma Bubbles Observed at Geomagnetically Conjugate Points Over the Brazilian Sector
Year2022
Access Date2024, May 09
Secondary TypePRE CI
2. Context
Author1 Silva, Diego Barros
2 Takahashi, Hisao
3 Wrasse, Cristiano Max
4 Figueiredo, Cosme Alexandre Oliveira Barros
5 Carrasco, Alexander José
Resume Identifier1
2 8JMKD3MGP5W/3C9JHCM
Group1 DICEP-CGCE-INPE-MCTI-GOV-BR
2 DICEP-CGCE-INPE-MCTI-GOV-BR
3 DICEP-CGCE-INPE-MCTI-GOV-BR
4 DICEP-CGCE-INPE-MCTI-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 bar_diego@hotmail.com
2
3 cristiano.wrasse@inpe.br
4 anagetinga@hotmail.com
Conference NameAGU Fall Meeting
Conference LocationChicago, IL
Date12-16 Dec. 2022
PublisherAGU
History (UTC)2022-12-13 17:59:53 :: simone -> administrator ::
2023-01-03 16:46:27 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractGround-based global navigation satellite systems (GNSS) receivers have been used to monitor the meridional (north-south) development of equatorial plasma bubbles (EPBs) at geomagnetically conjugate points over the Brazilian sector. EPBs were studied using detrended total electron content plots obtained from Boa Vista (MLat: 9.6°N), Itacoatiara (MLat: 3.3°N), Colíder (MLat: 5.0°S), and Cuiabá (MLat: 8.8°S) GNSS receivers. All GNSS receivers are located approximately under the same magnetic meridian. 655 nights with EPBs occurrence were analyzed using data from January 2012 to February 2016. In 459 nights (∼70%) the EPBs presented a symmetric development with respect to the geomagnetic equator. However, in 196 nights (∼30%) the EPBs presented an apparent asymmetry. The asymmetries are characterized as a displacement of the EPBs to north (or south) of the geomagnetic equator. The highest north (south) asymmetry occurrence was observed during December to January (March to April and September to October), and lowest during March to April and August to September (December to January). To investigate these asymmetries, we analyzed meridional wind data and used a numerical model to simulate the EPBs evolution. Both meridional wind data and numerical simulation results suggested that a trans-equatorial meridional wind blowing to north (south) would be able to cause a displacement of the EPBs to north (south) of the geomagnetic equator.
AreaCEA
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Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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