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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/CSTP6
Repositorysid.inpe.br/marciana/2004/07.26.11.05   (restricted access)
Last Update2004:07.26.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/07.26.11.05.34
Metadata Last Update2021:07.18.04.01.22 (UTC) administrator
Secondary KeyINPE-10991-PRE/6447
ISSN1364-6826
Citation KeyBatistaClemTokuLima:2004:StMeWi
TitleStructure of the mean winds and tides in the meteor region over Cachoeira Paulista, Brazil (22.7°S,45°W) and its comparison with models
Year2004
MonthApr.-June
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size114 KiB
2. Context
Author1 Batista, Paulo Prado
2 Clemesha, Barclay Robert
3 Tokumoto, A. S.
4 Lima, L. M.
Resume Identifier1 8JMKD3MGP5W/3C9JJ3H
2 8JMKD3MGP5W/3C9JGKH
Group1 DAE-INPE-MCT-BR
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume66
Number6-9
Pages623-636
History (UTC)2021-07-18 04:01:22 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsatmospheric tides
meteor radar
meteor region
mean winds
AbstractZonal and meridional winds in the region of the upper mesosphere and lower thermosphere (MLT) have been measured with a meteor radar at Cachoeira Paulista, Brazil (22.7°S, 45°W) during two years, from March 1999 to February 2001. Winds were calculated with temporal resolution of 1 h and vertical resolution of 2 km from 80 to 100 km height. Monthly means were calculated and the wind structure was decomposed into the mean, diurnal, semidiurnal and terdiurnal components. The mean wind showed the zonal component to dominate with westward wind above 90 km from May to October, a dominance of an eastward wind from October to April between 80 and 100 km and a small interannual variation. The meridional wind shows a simple structure with northward wind from October to April and Southward wind from May to September. The dominant mode in the diurnal tide has a wavelength ranging from 25 to 30 km, which is consistent with the S1,1 mode, in good agreement with the GWSM model. Large interannual variations and different phases were noted during November and December. The diurnal amplitudes are in general smaller than those predicted by the model, mainly during October. The semidiurnal amplitudes are in general, greater than those for the model, and the phases show some vertical propagation or are almost evanescent. The terdiurnal component although weak shows good height and interannual coherence.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Structure of the...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
Target Filescience.html
User Groupadministrator
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Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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