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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/3QTQTLH
Repositorysid.inpe.br/mtc-m21c/2018/04.18.16.37
Metadata Repositorysid.inpe.br/mtc-m21c/2018/04.18.16.37.04
Metadata Last Update2020:12.07.21.11.31 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyPiassiSilvPadi:2018:AnPcPc
TitleAnalysis of Pc3 and Pc4 magnetic pulsations in the South Atlantic Magnetic Anomaly region
Year2018
Access Date2024, May 18
Secondary TypePRE CI
2. Context
Author1 Piassi, Amanda Resende
2 Silva, Ligia Alves da
3 Padilha, Antônio Lopes
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JGJG
Group1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDGE-CGCEA-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)
Author e-Mail Address1 amanda.piassi@inpe.br
2 ligia.silva@inpe.br
3 antonio.padilha@inpe.br
Conference NameLatin American Conference on Space Geophysics, 11 (COLAGE)
Conference LocationBuenos Aires, Argentina
Date16-20 abr.
History (UTC)2018-04-18 16:37:04 :: simone -> administrator ::
2019-01-04 16:57:04 :: administrator -> simone :: 2018
2019-01-07 13:58:22 :: simone -> administrator :: 2018
2020-12-07 21:11:31 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractMuch of South America is aected by the South Atlantic Magnetic Anomaly (SAMA), characterized by the minimum intensity of the geomagnetic eld on the Earths surface. Due to the presence of this anomaly, there is an increase in particle precipitation from the internal radiation belt that surrounds the planet, generating dierent aeronomic eects. In this study, we investigated the eect of this process on the amplitude of Pc3-Pc4 magnetic pulsations as a function of the distance from the center of the anomaly. Data from highly sensitive uxgate magnetometers (1 Hz acquisition rate) operated by the Brazilian Space Weather Program (EMBRACE) and INTERMAGNET in several locations in South America are used in the analyzes. Four magnetic storms were selected during the year 2015 and data from 7 days before (quiet period) and 7 days after each storm (most disturbed period, including the recovery phase) were ltered in the Pc3-Pc4 intervals. The results show a permanent amplication in the pulsation amplitude at the station closest to the center of the anomaly. It is proposed that this amplication is linked to the increase of the ionospheric conductivity in SAMA, caused by the enhanced particle precipitation from the radiation belt. Also, this eect is continuous in the anomaly region, being valid for both low level geomagnetic activity (quiet days) and high level geomagnetic activity (disturbed days).
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Arrangementurlib.net > DIDGE > Analysis of Pc3...
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Next Higher Units8JMKD3MGPCW/3EU29DP
Host Collectionurlib.net/www/2017/11.22.19.04
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