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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/42NRRSL
Repositorysid.inpe.br/mtc-m21c/2020/06.26.12.39   (restricted access)
Last Update2020:06.26.12.39.53 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/06.26.12.39.53
Metadata Last Update2022:03.18.22.11.33 (UTC) administrator
DOI10.1051/swsc/2020022
ISSN2115-7251
Citation KeySousasantosAbSaBaSiLo:2020:CoLoOb
TitleFurther complexities on the pre-reversal vertical drift modeling over the Brazilian region: a comparison between long-term observations and model results
Year2020
Access Date2024, May 15
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size4004 KiB
2. Context
Author1 Sousasantos, Jonas
2 Abdu, Mangalathayil Ali
3 Santos, Angela
4 Batista, Inez Staciarini
5 Silva, André
6 Loures, Luis Eduardo
Resume Identifier1
2 8JMKD3MGP5W/3C9JHNK
3
4 8JMKD3MGP5W/3C9JHDA
Group1
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
3 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Tecnológico de Aeronáutica (ITA)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Tecnológico de Aeronáutica (ITA)
6 Instituto Tecnológico de Aeronáutica (ITA)
Author e-Mail Address1 jonasjss@ita.br
2 ma.abdu@inpe.br
3
4 inez.batista@inpe.br
JournalJournal of Space Weather and Space Climate
Volume10
Pagese2020022
Secondary MarkB5_GEOCIÊNCIAS
History (UTC)2020-06-26 12:40:30 :: simone -> administrator :: 2020
2022-03-18 22:11:33 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsPre-reversal vertical drift / Equatorial plasma electrodynamics / Ionospheric modeling
AbstractThe vertical component of the plasma drift, especially the evening-time pre-reversal drift, constitutes an important aspect of the nighttime electrodynamics of the equatorial ionosphere. Over the years, several studies using measurements and models have been performed to understand the characteristics of this process and its implications for the development of the instabilities leading to the plasma bubble formation and ionospheric scintillation. However, the Brazilian region presents some unique features that bring some difficulties for the vertical drift prognosis, which is required for the scintillation forecasting. These features are mainly related to the geomagnetic field lines topology that presents strong differences when compared to those of other equatorial longitudes. In this work, some of the difficulties for the prereversal vertical drift modeling and estimation are discussed; also, a dataset containing long-term observation (20012009) is compared with a widely used empirical model. The results show an intrinsic trend of underestimation by the model, which seems to be independent of latitude and seasonality thus suggesting an additional contribution arising from sources other than solely the geomagnetic topology. Also, the results indicate that the deviation can vary in the range of 040 m/s and the percentage error enhances with increasing values of pre-reversal vertical drift peak and reduces with increasing F10.7 values, thereby, indicating a clear possibility of meridional winds contribution which is not included in the empirical model used and may account for these differences.
AreaCEA
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4. Conditions of access and use
Languageen
Target FileSousasantos_Further.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/bibdigital/2013/10.12.21.02 5
sid.inpe.br/bibdigital/2013/09.29.20.43 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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