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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifierx6e6X3pFwXQZ3DUS8rS5/yy54w
Repositorycptec.inpe.br/walmeida/2003/06.24.14.11   (restricted access)
Last Update2005:01.31.02.00.00 (UTC) administrator
Metadata Repositorycptec.inpe.br/walmeida/2003/06.24.14.11.13
Metadata Last Update2021:02.10.18.59.14 (UTC) administrator
Secondary KeyINPE-9996-PRE/5556
ISSN0177-7971
Citation KeyRaoRosaBonaFran:2003:StFiWa
TitleStratospheric final warmings in the Southern Hemisphere and their energetics
Year2003
Secondary Date200303
Monthmar
Access Date2024, May 01
Secondary TypePRE PI
Number of Files1
Size945 KiB
2. Context
Author1 Rao, Vadlamudi Brahmananda
2 Rosa, Marcelo Barbio
3 Bonatti, José Paulo
4 Franchito, Sérgio Henrique
Resume Identifier1 8JMKD3MGP5W/3C9JJAJ
2 8JMKD3MGP5W/3C9JHNT
3 8JMKD3MGP5W/3C9JHJ7
4 8JMKD3MGP5W/3C9JJ82
Group1 DMD-INPE-MCT-BR
2 DMD-INPE-MCT-BR
3 DMD-INPE-MCT-BR
4 DMD-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais,(INPE/CPTEC)
2 Instituto Nacional de Pesquisas Espaciais(INPE/CPTEC)
3 Instituto Nacional de Pesquisas Espaciais(INPE/CPTEC)
4 Instituto Nacional de Pesquisas Espaciais(INPE/CPTEC)
Author e-Mail Address1 vbrao@cptec.inpe.br
2 marcelo@cptec.inpe.br
3
4 fran@cptec.inpe.br
e-Mail Addressdeicy@cptec.inpe.br
JournalMeteorology and Atmospheric Physics
Volume83
Number1-2
Pages35-49
History (UTC)2005-01-31 17:33:01 :: marciana -> administrator ::
2006-11-17 23:10:26 :: administrator -> marciana ::
2007-09-05 18:06:59 :: marciana -> administrator ::
2021-02-10 18:59:14 :: administrator -> marciana :: 2003
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsgeneral circulation model
troposphere
AbstractUsing 9 years (1985-1993) data, final stratospheric warmings in the Southern Hemisphere are studied. Interannual variations in the onset date and the temperatures are noted. In 1985 the stratosphere was colder by about 5 K and the wave activity was less. This year the final warming got delayed. In contrast in 1988 the final warming occurred earlier when compared with the mean picture and the wave activity was more. An examination of Eliassen-Palm fluxes showed the important role of planetary waves in the wave-mean flow interaction. In the energetics the most spectacular change is the reduction of zonal kinetic energy. Before the warming the energy exchanges were P-z --> P-e --> K-e --> K-z <-- P-z and after the warming they were P-z <-- P-e <-- K-e --> K-z <-- P-z. The dramatic reduction of zonal kinetic energy seems to be due to two effects: the reduction in K-e --> K-z conversion and the weakening of direct meridional circulation.
AreaMET
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMD > Stratospheric final warmings...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileRao_Stratospheric final.pdf
User Groupadministrator
marciana
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/43SKC35
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectioncptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
NotesDoi:10.1007/s00703-002-0558-6
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi format isbn label lineage mark mirrorrepository nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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