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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/39RQ935
Repositorydpi.inpe.br/plutao/2011/06.11.02.29
Last Update2011:07.25.14.29.48 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2011/06.11.02.29.09
Metadata Last Update2018:06.05.00.01.16 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.5194/angeo-29-209-2011
ISSN0992-7689
Labellattes: 8030262077949409 10 BagestonWHBGTFAFN:2011:CaStMe
Citation KeyBagestonWHBGTFAFDN:2011:CaStMe
TitleCase study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
ProjectNational Science Foundation OPP-0438777 - CNPq[305923/2008-0, 304277/2008-8]
Year2011
Access Date2024, May 22
Secondary TypePRE PI
Number of Files1
Size1148 KiB
2. Context
Author 1 Bageston, José Valentin
 2 Wrasse, C. M.
 3 Hibbins, R. E.
 4 Batista, Paulo Prado
 5 Gobbi, D.
 6 Takahashi, H.
 7 Fritts, D. D.
 8 Andrioli, Vânia Fátima
 9 Fechine, J.
10 Denardini, C. M.
11 Nardin, Clezio Marcos De
Resume Identifier 1
 2
 3
 4 8JMKD3MGP5W/3C9JJ3H
 5
 6
 7
 8
 9
10
11 8JMKD3MGP5W/3C9JGSH
Group 1 DAE-CEA-INPE-MCT-BR
 2
 3
 4 DAE-CEA-INPE-MCT-BR
 5 DAE-CEA-INPE-MCT-BR
 6 DAE-CEA-INPE-MCT-BR
 7
 8 DAE-CEA-INPE-MCT-BR
 9
10 DAE-CEA-INPE-MCT-BR
11 DAE-CEA-INPE-MCT-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 VSE, Sao Jose Dos Campos, Brazil
 3 BAS, Cambridge, England
 4 Norwegian Univ Sci & Technol, N-7034 Trondheim, Norway
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 NWRA, CoRA, Boulder, CO USA
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Univ Fed Campina Grande, Campina Grande, Brazil
10 Univ Fed Campina Grande, Campina Grande, Brazil
11 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 bageston@gmail.com
 2
 3
 4 ppbatista@laser.inpe.br
 5
 6
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 8 vania@laser.inpe.br
 9
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11 denardin@dae.inpe.br
e-Mail Addressdenardin@dae.inpe.br
JournalAnnales Geophysicae
Volume29
Number1
Pages209-219
Secondary MarkB3_ASTRONOMIA_/_FÍSICA B1_GEOCIÊNCIAS
History (UTC)2011-06-11 17:43:42 :: lattes -> administrator :: 2011
2011-07-25 14:21:53 :: administrator -> marciana :: 2011
2011-07-25 14:29:48 :: marciana -> administrator :: 2011
2011-07-26 03:17:03 :: administrator -> marciana :: 2011
2011-08-03 12:33:12 :: marciana -> administrator :: 2011
2011-08-22 07:25:04 :: administrator -> marciana :: 2011
2011-11-10 12:59:55 :: marciana -> administrator :: 2011
2011-11-11 18:06:32 :: administrator -> tereza@sid.inpe.br :: 2011
2011-11-17 17:00:16 :: tereza@sid.inpe.br -> banon :: 2011
2011-11-23 13:37:41 :: banon -> administrator :: 2011
2018-06-05 00:01:16 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAirglow
Aurora
Middle Atmosphere Dynamics
Waves and Tides
GRAVITY-WAVE EVENT
LIDAR OBSERVATION
BORE EVENT
MF RADAR
OH
CLIMATOLOGY
LATITUDES
CAMPAIGN
REGION
TIDES
AbstractOn 16-17 July 2007 during an observational campaign at Comandante Ferraz Antarctic Station (62 degrees S, 58 degrees W), a mesospheric wall was observed with an airglow all-sky imager. The wave appeared like an extensive dark region in the all-sky airglow images, with a large depletion in the OH emission. Simultaneous mesospheric winds measured with a MF radar at Rothera station and temperature profiles from SABER instrument, on board of TIMED satellite, were used to obtain the propagation condition of the wave. Wind measurements during four days, around the time of observation of the wave, are presented in order to discuss the type and consistence of the duct in which this wave was propagating. By using wavelet analysis and tidal amplitude components we found that 12 and 8 h components were the most important periodicities around the time interval of the wave observation. A collocated imaging spectrometer, for mesospheric temperature measurements, has been operated simultaneously with the all-sky imager. Direct effects of the mesospheric front have been seen in the spectrometric measurements, showing an abrupt decrease in both OH intensity and rotational temperature when the wave front passes overhead. The main contribution of the present work is the investigation of the type of duct in which the wall event was propagating. We found evidences for a thermal duct structure to support the mesospheric wall propagation. This result was obtained by two types of analysis: (a) the tidal components analysis and winds filtering (harmonic analysis), and (b) comparison between the terms of the m(2) dispersion relation.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Case study of...
doc Directory Contentaccess
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4. Conditions of access and use
data URLhttp://plutao.sid.inpe.br/ibi/J8LNKAN8RW/39RQ935
zipped data URLhttp://plutao.sid.inpe.br/zip/J8LNKAN8RW/39RQ935
Languageen
Target Fileangeo-29-209-2011.pdf
User Groupadministrator
banon
lattes
marciana
tereza@sid.inpe.br
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/bibdigital/2013/09.29.20.43 3
sid.inpe.br/mtc-m21/2012/07.13.14.44.03 1
URL (untrusted data)http://www.ann-geophys.net/29/209/2011/
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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7. Description control
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