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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3PDMP32
Repositorysid.inpe.br/mtc-m21b/2017/08.08.18.45
Last Update2017:08.08.18.45.51 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/08.08.18.45.51
Metadata Last Update2018:06.04.02.27.38 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyMoraesPaulPaulBati:2017:EvLuTi
TitleEvidence of the lunar tide in the ionosphere
Year2017
Access Date2024, May 14
Secondary TypePRE CI
Number of Files1
Size2280 KiB
2. Context
Author1 Moraes, Joyrles Fernandes
2 Paulino, Ana Roberta
3 Paulino, Igo
4 Batista, Inez Staciarini
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHDA
Group1
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Federal de Campina Grande (UFCG)
2 Universidade Federal de Campina Grande (UFCG)
3 Universidade Federal de Campina Grande (UFCG)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4 inez.batista@inpe.br
Conference NameInternational Congress of the Brazilian Geophysical Sociey, 15
Conference LocationRio de Janeiro, RJ
Date31 jul. - -3 ago.
History (UTC)2017-08-08 18:46:31 :: simone -> administrator :: 2017
2018-06-04 02:27:38 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractUsing data collected by a Digisonde DPS-04 located at Cachoeira Paulista SP, it was possible to identify the lunar tide in the ionosphere. We have used two parameters (fof2 and hmf2) during 2001 in order to study the semidiurnal and diurnal lunar tide. The amplitude and phase of these oscillations were calculated using least square analysis. The diurnal tide presented a maximum amplitude of 0.25 MHz in Fof2 and 6 km in Hmf2. The phase was ranged between -1 and 1 rad. Both parameters presented a seasonal variation in phase and amplitude. For the Semidiunal lunar tide the maximum amplitude was 0.25 MHz in August for fof2, and 4.5 km for hmF2 in June. A semiannual variation was observed as well.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Evidence of the...
doc Directory Contentaccess
source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://mtc-m21b.sid.inpe.br/ibi/8JMKD3MGP3W34P/3PDMP32
zipped data URLhttp://mtc-m21b.sid.inpe.br/zip/8JMKD3MGP3W34P/3PDMP32
Languageen
Target Filemoraes_evidence.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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7. Description control
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