Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/iris@1916/2005/12.19.13.09   (restricted access)
Last Update2005:12.19.13.09.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/12.19.13.09.41
Metadata Last Update2018:06.05.01.16.35 (UTC) administrator
Secondary KeyINPE--13222-PRE/8478
ISSN0273-1177
Citation KeyTakahashiNaShTsLiGo:2005:AiOHEm
TitleAirglow OH emission height inferred from the OH temperature and meteor trail diffusion coefficient
Year2005
Access Date2024, May 08
Secondary TypePRE PI
Number of Files1
Size160 KiB
2. Context
Author1 Takahashi, Hisao
2 Nakamura, T.
3 Shiokawa, K.
4 Tsuda, T.
5 Lima, L. M.
6 Gobbi, Delano
Resume Identifier1 8JMKD3MGP5W/3C9JHCM
2
3
4
5
6 8JMKD3MGP5W/3C9JGTE
Group1 DAE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Aeronomia (INPE, DAE)
JournalAdvances in Space Research
Volume35
Number11
Pages1940-1944
History (UTC)2006-01-18 17:59:31 :: simone -> administrator ::
2012-07-17 12:41:15 :: administrator -> simone ::
2012-10-03 14:53:09 :: simone -> administrator :: 2005
2018-06-05 01:16:35 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAirglow OH emission height
Meteor diffusion
OH temperature
AbstractSimultaneous observations of the airglow OH(6,2) band rotational temperature, TOH, and meteor trail ambipolar diffusion coefficient, D, were carried out at Shigaraki (35°N, 136°E), during PSMOS 2003 Campaign, January 28 to February 8, 2003. The OH emission height was estimated by cross correlation analysis of the TOH and D nocturnal variations. A good correlation between TOH and D was obtained at 85 km of altitude. From the nocturnal variations of TOH and D, it is found that the OH emission peak height varied from 88 km before the midnight to 84 km in the early morning. The height variation could be caused by an atmospheric tidal effect in the emission height.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Airglow OH emission...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Target Filetakahashi.pdf
User Groupadministrator
simone
Reader Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.44.27 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format identifier isbn label language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
update 


Close