Close

1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/H37DF
Repositorysid.inpe.br/iris@1905/2005/08.02.21.48.28   (restricted access)
Last Update2013:04.01.17.57.43 (UTC) jefferson
Metadata Repositorysid.inpe.br/iris@1905/2005/08.02.21.48.30
Metadata Last Update2018:06.06.03.53.46 (UTC) administrator
Secondary KeyINPE-8643-PRE/4377
ISSN0273-1177
Label9617
Citation KeyMedeirosTayTakBatGob:2001:AnAiWa
TitleAn anusual airglow wave event observed at Cachoeira Paulista 23 degree S
Year2001
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size5267 KiB
2. Context
Author1 Medeiros, Amauri Fragoso de
2 Taylor, Michael J.
3 Takahashi, Hisao
4 Batista, Paulo Prado
5 Gobbi, Delano
Group1 DAE-INPE-MCT-BR
2
3 DAE-INPE-MCT-BR
4 DAE-INPE-MCT-BR
5 DAE-INPE-MCT-BR
JournalAdvances in Space Research
Volume27
Number10
Pages1749-1754
History (UTC)2013-04-01 17:57:12 :: administrator -> jefferson :: 2001
2013-04-01 17:57:43 :: jefferson -> administrator :: 2001
2018-06-06 03:53:46 :: administrator -> marciana :: 2001
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAERONOMIA
ondas de gravidade
aeroluminescencia
gravity waves
airglow
AbstractAn all-sky CCD airglow imager has been used to obtain a wealth of data on the MLT airglow emissions from Cachoeira Paulista, Brazil (22.7 degrees S, 45.0 degrees W). Measurements of the NIR OH, OI(557.7 nm), O2(0,1)and the thermospheric OI(630.0 nm)emissions have been made since October 1998. In addition, simultaneous measurements of the airglow zenith intensities and rotational temperatures, and vertical wind structure between 80 and 100 km were made using a co-located multi-channel photometer and a meteor radar. On the night of July 13, 1999, the CCD images showed active wave events exhibiting a variety of short period wave structures. The activity started with ripple patterns over the whole sky, lasting for almost one hour. Later the patterns changed to extensive band-like structures that lasted for several hours. After local midnight a bore-like wave-front passed overhead propagating towards the North. When the front was in the zenith the image data showed an increase in both the OI (5577 nm)and O2 (0,1)emissions, whilst a decrease in the OH intensity was observed, which is opposite to that observed by Taylor et al., (1995a). The co-located photometer revealed an exceptionally large intensity (>40) and temperature (similar to 12) perturbation throughout the night that appears to be associated with a large-scale gravity wave perturbation with significant vertical phase shift between the different emissions.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > An anusual airglow...
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-S0273117701003179-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
Empty Fieldsaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
update 


Close