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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/3SETCHP
Repositorysid.inpe.br/mtc-m21c/2018/12.27.10.29
Last Update2020:09.30.12.57.46 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2018/12.27.10.29.38
Metadata Last Update2020:09.30.12.57.47 (UTC) simone
Secondary KeyINPE--PRE/
Citation KeyTsali-BrownPauLimBatBat:2018:EfLuTi
TitleEffects of lunar tides in the F region of the ionosphere
Year2018
Access Date2024, May 16
Secondary TypePRE CN
Number of Files1
Size171 KiB
2. Context
Author1 Tsali-Brown, Vera Yesutor
2 Paulino, Ana Roberta
3 Lima, L. M.
4 Batista, Inez Staciarini
5 Batista, Paulo Prado
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHDA
5 8JMKD3MGP5W/3C9JJ3H
Group1
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
5 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Estadual da Paraíba (UEPB)
2 Universidade Estadual da Paraíba (UEPB)
3 Universidade Estadual da Paraíba (UEPB)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 yesutor4@yahoo.com
2
3
4 inez.batista@inpe.br
5 paulo.batista@inpe.br
Conference NameSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 7 (SBGEA)
Conference LocationSanta Maria, RS
Date05-09 nov
History (UTC)2018-12-27 10:29:38 :: simone -> administrator ::
2019-01-14 17:06:41 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe effect of the lunar tide in the F region of the Brasilian ionosphere was studied in this work using measurements provided by the ionosonde installed in Cachoeira Paulista (22.7 ° S, 45.0 ° W) from 2009 to 2011. To identify the variations associated with the lunar tides, the following parameters were used: height of maximum density of the F2 region (hmF2) and the critical frequency of the F2 (foF2) region. The influence of the lunar tide in the ionosphere was then obtained using the residual measurements which were calculated by removing the influence of the solar tides for each day. The solar time of the measurements were also converted to lunar time. In order to obtain the monthly amplitudes and phases of the lunar tide components, harmonic analysis was performed. The maximum amplitude value obtained in foF2 was ~ 0.41MHz for the diurnal component and ~0.42MHz for the semidiurnal component. Also the maximum amplitude value obtained in hmF2 was ~6.25 km for the diurnal component and ~7.76 km for the semidiurnal component. The seasonal variations for the amplitudes in foF2 and hmF2 exhibited annual and semiannual patterns.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Effects of lunar...
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source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3SETCHP
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3SETCHP
Languagept
Target Filetsali_effects.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.58 5
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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