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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/3SB3ATS
Repositorysid.inpe.br/mtc-m21c/2018/12.03.12.04
Last Update2020:12.29.15.10.06 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2018/12.03.12.04.27
Metadata Last Update2020:12.29.15.10.07 (UTC) simone
Secondary KeyINPE--PRE/
Citation KeyPaulaMCNBMCAM:2018:IoAmSc
TitleIonospheric amplitude scintillation behavior over the low latitude station of São Luís during the September 6 to 10, 2017 magnetic storm
Year2018
Access Date2024, May 16
Secondary TypePRE CI
Number of Files1
Size74 KiB
2. Context
Author1 Paula, Eurico Rodrigues de
2 Moraes, Alison de Oliveira
3 Caton, Ron
4 Negreti, Patrícia Mara de Siqueira
5 Batista, Inez Staciarini
6 Martinon, André Ricardo Fazanaro
7 Cunha Neto, Acácio
8 Abdu, Mangalathayil Ali
9 Monico, João Francisco Galera
Resume Identifier1 8JMKD3MGP5W/3C9JH2U
2
3
4
5 8JMKD3MGP5W/3C9JHDA
6
7
8 8JMKD3MGP5W/3C9JHNK
Group1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
5 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
6 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
7 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
8 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto de Aeronáutica e Espaço (IAE)
3 Air Force Research Laboratory
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
8 Instituto Nacional de Pesquisas Espaciais (INPE)
9 Universidade Estadual Paulista (UNESP)
Author e-Mail Address1 eurico.paula@inpe.br
2
3
4 patricia.negreti@inpe.br
5 inez.batista@inpe.br
6 andre.martinon@inpe.br
7 acacio.cunha@inpe.br
8 ma.abdu@inpe.br
Conference NameAGU Fall Meeting
Conference LocationWashington, D. C.
Date10-14 dec.
History (UTC)2018-12-03 12:04:28 :: simone -> administrator ::
2019-01-04 16:57:14 :: administrator -> simone :: 2018
2019-01-07 12:14:00 :: simone -> administrator :: 2018
2019-01-14 17:06:39 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe September 6 to 10, 2017 magnetic storm was caused by an X9 solar flare followed by a CME and the maximum Sym H magnetic index reached a value of -146 nT at 01:08 UT on day 08, after a Bz southward incursion of -31.21nT at 23:31 UT on day 07 and the Kp magnetic index reached 8. The solar wind increased from 400 km/s to about 600 km/s around 24 UT of day 06 and to about 800 km/s in the following night of 07/08. During the recovery phase of this storm there was another Bz southward incursion of -17.46 nT at 11:55 UT on day 08 when Sym H reached -115 nt at 13:56 UT and Kp reached the value of 8.33. In this work the ionospheric amplitude scintillation at São Luís (02.5o S, 44.3 o W, dip lat -04.67 o) was studied using data from an AFRL/INPE VHF receiver and a CIGALA/CALIBRA Septentrio receiver, both installed at São Luís. The vertical plasma drift during daytime hours was determined using the magnetometer data from Belém (1.5 o S, 48.5 o W, dip lat -1.12 o) and Petrolina (09.4 o S, 40.5 o W, dip lat -13.45 o) and that during the evening prereversal enhancement period was calculated using ionogram data from the São Luís digisonde. Compared to the geomagnetically quiet days of September 2017, both VHF and GNSS S4 scintillation indices presented an increase during the night of 07/08 when there was a strong increase in the vertical plasma drift due to a prompt penetration under-shielding electric field of eastward polarity (Ey) of about 17 mV/m magnitude. In contrast to this, on the night of 08/09 the ionospheric scintillation was completely inhibited as is a typical response to a disturbance dynamo electric field of westward polarity. During the following nights scintillation events were again gradually observed. Another Ey increase was observed at about 12 UT (09 LT) on day 08 when no scintillation was normally observed since it was daytime. The zonal drift determined by the VHF receiver around 24 UT (21 LT) was about 100 m/s and 150 m/s eastward on the nights of 05/ 06 and 06/07, respectively. However, during the night of 07/08 of the storm, the zonal drift reversed to westward with a velocity of about -80 m/s. After the storm period the zonal drifts became eastward.
AreaCEA
ArrangementIonospheric amplitude scintillation...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3SB3ATS
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3SB3ATS
Languageen
Target Filepaula_ionospheric.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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