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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3PJ5DN2
Repositorysid.inpe.br/mtc-m21b/2017/09.04.19.30
Last Update2017:09.04.19.30.46 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/09.04.19.30.46
Metadata Last Update2018:06.04.02.27.49 (UTC) administrator
DOI10.1002/2017JA024052
ISSN2169-9402
Citation KeyPaulinoLABBPTW:2017:LuTiTo
TitleLunar tides in total electron content over Brazil
Year2017
MonthJuly
Access Date2024, May 09
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size20096 KiB
2. Context
Author1 Paulino, A. R.
2 Lima, L. M.
3 Almeida, S. L.
4 Batista, Paulo Prado
5 Batista, Inez Staciarini
6 Paulino, I.
7 Takahashi, Hisao
8 Wrasse, Cristiano Max
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ3H
5 8JMKD3MGP5W/3C9JHDA
6
7 8JMKD3MGP5W/3C9JHCM
Group1
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
5 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
6
7 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
8 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)
6 Universidade Federal de Campina Grande (UFCG)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
8 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4 paulo.batista@inpe.br
5 inez.batista@inpe.br
6
7
8 cristiano.wrasse@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume122
Number7
Pages7519-7529
History (UTC)2017-09-04 19:30:46 :: simone -> administrator ::
2017-09-04 19:30:46 :: administrator -> simone :: 2017
2017-09-04 19:31:28 :: simone -> administrator :: 2017
2018-06-04 02:27:49 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordslunar tides
ionosphere
TEC
AbstractUsing data from Global Navigation Satellite Systems dual frequency receivers, the lunar tides were studied in the ionospheric total electron content (TEC) over Brazil from 2011 to 2014. In order to calculate the amplitudes and phases of the lunar tides, quiet magnetic days within a 27 day (window) have been used to remove the solar rotation effects. Relative residuals TEC were calculated by performing a spectral analysis by removing the solar tide contributions. Lastly, a lunar month size window was used to calculate the amplitude and phase of the lunar components. Lunar diurnal tide amplitudes showed a semiannual variation with maximum in the equinox months for almost all latitudes, while lunar semidiurnal amplitudes were larger in December and January and may be related to sudden stratospheric warming events. Both components did not display significant longitudinal variation what could be due to the short range of longitude (30 degrees). Lunar diurnal amplitudes were basically uniform over Brazil, while lunar semidiurnal amplitudes showed some peaks over the equatorial ionization anomaly crest and minimum values near the magnetic equator.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Lunar tides in...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 04/09/2017 16:30 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34P/3PJ5DN2
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34P/3PJ5DN2
Languageen
Target Filepaulino_lunar.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.49.58 1
sid.inpe.br/bibdigital/2013/09.29.20.43 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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