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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/3QTQQES
Repositorysid.inpe.br/mtc-m21c/2018/04.18.15.58
Metadata Repositorysid.inpe.br/mtc-m21c/2018/04.18.15.58.27
Metadata Last Update2020:12.07.21.11.30 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyDamascenoCorrMach:2018:MuObIo
TitleMulti-instrument observations of the ionospheric response to the 7 September 2017 geomagnetic storm in the South American Sector
Year2018
Access Date2024, May 16
Secondary TypePRE CI
2. Context
Author1 Damasceno, Gabriel Campos
2 Correia, Emília
3 Macho, Eduardo Perez
Resume Identifier1
2 8JMKD3MGP5W/3C9JH2C
Group1
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Presbiteriana Mackenzie
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Presbiteriana Mackenzie
Author e-Mail Address1
2 emilia.correia@inpe.br
Conference NameLatin American Conference on Space Geophysics, 11 (COLAGE)
Conference LocationBuenos Aires, Argentina
Date16-20 abr.
History (UTC)2018-04-18 15:58:44 :: simone -> simone] :: 2018
2018-04-18 15:58:44 :: simone] -> administrator :: 2018
2020-12-07 21:11:30 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe South American ionospheric behavior during the period from 05 to 10 September 2017 is investigated using data from GNSS network from Continuous Monitoring Brazilian Network (RBMC) and ionosondes available in the Space Weather Brazilian Studying and Monitoring (Embrace) site. The geomagnetic activity was produced by the impact of two Coronal Mass Ejections (CMEs) on the Earth magnetosphere . The first one caused a geomagnetic storm that started at 19:00 UT on 07 September and reached the maximum at 02:00 UT on 08 September with DST Index of -142 nT (Intense Storm), KP index 8 and Auroral index 1500 nT. During the recovering phase of this storm another CME arrived at 11:00 UT on 08 September increasing the geomagnetic activity, with Dst reaching -122 nT at 15:00 UT. The Vertical Total Electron Content (VTEC) measured at different latitudes shows a distinct ionospheric response to each storm phase. During the onset main phase of the geomagnetic storm on 7 September VTEC increased at equatorial latitudes during afternoon, and after sunset shows another increase as consequence of electricfield associated with the evening Pre-reversal Enhancement (PRE). In association with the intensification of magnetic storm on 8 September, the VTEC shows an increase during sunrise and the fountain effect was intensified. The results shows that during the first hours of the main phase geomagnetic storm the ionospheric response was mainly affected by the prompt penetration electric fields (PPEFs), being a combination of PPEF and dynamo effects afterwards.
AreaCEA
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Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Host Collectionurlib.net/www/2017/11.22.19.04
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