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1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/GT5tC
Repositorysid.inpe.br/iris@1905/2005/07.26.22.40.49   (restricted access)
Last Update2013:04.02.11.54.57 (UTC) jefferson
Metadata Repositorysid.inpe.br/iris@1905/2005/07.26.22.40.57
Metadata Last Update2018:06.06.04.11.33 (UTC) administrator
Secondary KeyINPE-4720-PRE/1397
ISSN0273-1177
Label2886
Citation KeyClemesha:1990:ObTh
TitleStratification processes in the atmospheric sodium layer: observations and theory
Year1990
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size780 KiB
2. Context
AuthorClemesha, Barclay Robert
GroupDAE-INPE-BR
JournalAdvances in Space Research
Volume10
Number10
Pages(10)59-(10)70
History (UTC)2013-04-02 11:54:30 :: administrator -> jefferson :: 1990
2013-04-02 11:54:57 :: jefferson -> administrator :: 1990
2018-06-06 04:11:33 :: administrator -> marciana :: 1990
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAERONOMIA
ATMOSPHERIC LASERS
ATMOSPHERIC TIDES
SODIUM LAYER
AbstractThe mechanisms responsible for the formation of the alkali metal layers seem to be quite different in nature to those responsible for other atmospheric layers. In discussing the sodium layer in this context we must include both the mechanisms responsible for its basic production and the phenomena which produce structures within the layer. Although there is little doubt that the sodium layer owes its origin to the deposition into the atmosphere of extra-terrestrial material, how this deposition leads to the formation of a narrow layer of free sodium atoms is still an open question. With respect to the formation of structures within the layer it is clear that tides and gravity waves play an important role, although there can be little doubt that other factors are also at work. Of particular interest is the observation of thin layers having peak densities about an order of magnitude greater than normal, and a width an order of magnitude less. A number of mechanisms for the formation of these layers have been discussed in the literature, including direct meteor deposition, ion layer formation via the windshear mechanism, and evaporation from aerosol layers. None of these mechanisms has been analysed in detail, however, and the origin of these layers is still open to debate.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Stratification processes in...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File1-s2.0-027311779090010W-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
NotesCOSPAR-ESPOO, 27, 18-29 July, 1988, Helsinkei, FI.
Empty Fieldsaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn lineage mark mirrorrepository month nextedition 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
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