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1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/GUKJ5
Repositorysid.inpe.br/iris@1905/2005/07.29.22.40.40   (restricted access)
Last Update2013:04.02.11.34.01 (UTC) jefferson
Metadata Repositorysid.inpe.br/iris@1905/2005/07.29.22.40.48
Metadata Last Update2018:06.06.04.03.54 (UTC) administrator
Secondary KeyINPE-8328-PRE/4111
ISSN0273-1177
Label9299
Citation KeyTakahashiGoBaMeTeBu:1998:DyInEq
TitleDynamical influence on the equatorial airglow observed from the South American Sector
Year1998
Secondary Date20010724
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size3981 KiB
2. Context
Author1 Takahashi, Hisao
2 Gobbi, Delano
3 Batista, Paulo Prado
4 Melo, S. M. L.
5 Teixeira, Nelson Rodrigues
6 Buriti, R. A.
Group1 DAE-INPE-MCT-BR
2 DAE-INPE-MCT-BR
3 DAE-INPE-MCT-BR
4
5 DAE-INPE-MCT-BR
JournalAdvances in Space Research
Volume21
Number6
Pages817-825
History (UTC)2013-04-02 11:33:07 :: administrator -> jefferson :: 1998
2013-04-02 11:34:01 :: jefferson -> administrator :: 1998
2018-06-06 04:03:54 :: administrator -> marciana :: 1998
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAERONOMIA
America do Sul
emissao atmosférica
ondas
mares
luminescência
atmosférica equatorial
atmospheric emission
tides (tidal oscillation)
equatorial atmosphere
airglow (atmosphere emission)
AbstractThe upper atmospheric airglow emissions, OI 557.7 nm, NaD 589.3 nm, OH (9,4) and O2 atmospheric (0,1) bands and their rotational temperatures have been measured using ground-based multichannel airglow photometers, one located near the equator at Fortaleza (3.9 S, 38.4 W) and the other at low-middle latitude Cachoeira. Paulista (22.7 S, 45.0 W). Monthly averaged nocturnal variations calculated from the data from 1987 to 1993 were used to study the influence of atmospheric dynamical processes on these emissions. Harmonic analysis revealed that the Cachoeira Paulista data are mainly represented 12 hour period oscillation. Phase differences between the different emissions reveal that the vertical phase velocity is about 4 km/h and the vertical wavelength about 50 km. Fortaleza data on the other f. showed longer period, 24 hours, slow vertical propagation velocity, 1.1 km/h, and short veil wavelength, about 30 km. These facts lead us to conclude that the Cachoeira Paulista data are mainly controlled by the semidiurnal tidal oscillation and the Fortaleza data are controlled by the diurnal tide.
AreaCEA
ArrangementDynamical influence on...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File1-s2.0-S0273117798001112-main.pdf
User Groupadministrator
jefferson
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
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7. Description control
e-Mail (login)marciana
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