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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/3RFJS7L
Repositorysid.inpe.br/mtc-m21c/2018/07.18.13.51
Last Update2020:12.29.12.28.20 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2018/07.18.13.51.29
Metadata Last Update2020:12.29.12.28.21 (UTC) simone
Secondary KeyINPE--PRE/
Citation KeyPaulinoPBFLBBB:2018:LuTiIo
TitleThe lunar tides in the ionosphere over brazil
Year2018
Access Date2024, May 16
Secondary TypePRE CI
Number of Files1
Size62 KiB
2. Context
Author1 Paulino, Ana Roberta
2 Paulino, Igo
3 Brown, Vera
4 Fernades, Joyrles
5 Lima, Lourivaldo
6 Buriti, Ricardo
7 Batista, Paulo Prado
8 Batista, Inez Staciarini
Resume Identifier1
2
3
4
5
6
7 8JMKD3MGP5W/3C9JJ3H
8 8JMKD3MGP5W/3C9JHDA
Group1
2
3
4
5
6
7 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
8 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Estadual da Paraíba (UEPB)
2 Universidade Federal de Campina Grande (UFCG)
3 Universidade Estadual da Paraíba (UEPB)
4 Universidade Federal de Campina Grande (UFCG)
5 Universidade Estadual da Paraíba (UEPB)
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 arspaulino@gmail.com
2 igopaulino@gmail.com
3 yesutor4@yahoo.com
4 joyrles1996@gmail.com
5 lourivaldo_mota@yahoo.com.br
6 rburiti@df.ufcg.edu.br
7 paulo.batista@inpe.br
8 inez.batista@inpe.br
Conference NameCospar Scientific Assembly, 42
Conference LocationPasadena, California
Date14-22 July
History (UTC)2018-07-18 13:52:34 :: simone -> administrator :: 2018
2019-01-18 02:41:36 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe atmospheric lunar tide is excited by gravitational action in the lower atmosphere and by the movement of the oceans and Earths surface. Due to the fact that the source of the lunar tide does not change, the determination of this oscillation in the ionosphere is an excellent tool for understanding the coupling mechanism between the neutral and ionized atmospheres. The lunar tide has been studied in the mesosphere-thermosphere-ionosphere in different longitudinal sectors and using different observational techniques and simulations. However, there are some aspects of lunar tide that still need explanation, for example, the temporal variability of this oscillation. So, in this work, the diurnal and semidiurnal lunar tides are investigated in the ionosphere using ionosonde data over Brazil. The ionosonde measurements were collected at Cachoeira Paulista (22.7° S; 45.0° W) and São Luis (2.6° S; 44° W) from 2001 to 2009 with a temporal resolution of 15 minutes. Using these data, it was possible to extract the characteristics of the lunar tide. Salient features of this oscillation are presented and discussed in this work. For instance, the semidiurnal lunar tide is dominant comparing to the diurnal tide and had amplitude of 0.6 MHz in foF2 and 7 km in hmF2.
AreaCEA
ArrangementThe lunar tides...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 18/07/2018 10:51 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3RFJS7L
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3RFJS7L
Languageen
Target Filepaulino_lunar.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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7. Description control
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