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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/44D5SQL
Repositorysid.inpe.br/mtc-m21c/2021/03.25.18.30
Metadata Repositorysid.inpe.br/mtc-m21c/2021/03.25.18.30.49
Metadata Last Update2022:04.03.19.25.20 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyConceiçãoSantosMuReFaAnBaCa:2021:RoTiWi
TitleOn the role of tidal winds in the descending of the high type of sporadic layer (Esh)
Year2021
Access Date2024, May 18
Secondary TypePRE CN
2. Context
Author1 Conceição Santos, F.
2 Muella, M. T. A. H.
3 Resende, Laysa Cristina Araújo
4 Fagundes, P. R.
5 Andrioli, Vania Fátima
6 Batista, Paulo Prado
7 Carrasco, A. J.
Resume Identifier1
2
3
4
5
6 8JMKD3MGP5W/3C9JJ3H
Group1
2
3 DICEP-CGCE-INPE-MCTI-GOV-BR
4
5 CGCE-CGCE-INPE-MCTI-GOV-BR
6 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade do Vale do Paraíba (UNIVAP)
2 Universidade do Vale do Paraíba (UNIVAP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidade do Vale do Paraíba (UNIVAP)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3 laysa.resende@gmail.com
4
5 vaniafatima@gmail.com
6 paulopradobatista@yahoo.com
Conference NameSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA)
Conference LocationOnline
Date22-26 mar.
History (UTC)2021-03-25 18:30:49 :: simone -> administrator ::
2022-04-03 19:25:20 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractAs the prevailing tidal winds in the E region are generated by heating mechanisms, the dynamics of Es layers impacted by solar tides is a relevant theme in the space weather studies. This paper aims to identify the tidal wind component involved in the mechanism of formation and descending of the high type of sporadic layer (Esh). The Esh layers observed at altitudes between around 120 and 150 km in the Brazilian low latitude stations of Jata´ı and Sao Jos´e dos Campos during the months of April, June, September and December of 2016 are used in this analysis. The height variability and altitude descent of the Esh layers are analyzed from the hEs parameter obtained by ionosonde data. In this study, the observational data are compared with the simulations generated by an extended version of the Ionospheric E- Region Model (MIRE). At higher altitudes in the E region, the results show that the prevailing tidal pattern and wind direction controlling the Esh layer formation and descent are different depending on month: (a) in April and June the zonal wind component and the associated semidiurnal tidal oscillations prevail, with some differences in terms of time of occurrence and descending speeds, and (b) in September and December the diurnal tidal periodicities become dominant, and both the meridional and zonal wind components seem to control the descending of the Esh layers. Since the role of the tidal periodicities and wind directions changed depending on the month, the results suggest a possible seasonal tidal wind pattern, which is not well understood from the present study but requires further investigation.
AreaCEA
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4. Conditions of access and use
Languageen
User Groupsimone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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