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1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/H37x5
Repositorysid.inpe.br/iris@1905/2005/08.02.21.42.35   (restricted access)
Last Update2005:09.05.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1905/2005/08.02.21.42.37
Metadata Last Update2018:06.06.03.53.31 (UTC) administrator
Secondary KeyINPE-8473-PRE/4238
ISSN0273-1177
Label9460
Citation KeyPimentaFBSGMTT:2001:MeUsOI
TitleIonospheric plasma bubble zonal drift: A methodology using OI 630 nm all-sky imaging systems
Year2001
Secondary Date20011107
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size396 KiB
2. Context
Author1 Pimenta, A. A.
2 Fagundes, Paulo Roberto
3 Bittencourt, José Augusto
4 Sahai, Yogeshwar
5 Gobbi, Delano
6 Medeiros, Amauri Fragoso de
7 Taylor, Michael J.
8 Takahashi, Hisao
Group1 DAE-INPE-MCT-BR
2 DGE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
JournalAdvances in Space Research
Volume27
Number6-7
Pages1219-1224
History (UTC)2005-08-02 21:42:38 :: administrator -> jefferson ::
2005-09-05 15:46:24 :: jefferson -> administrator ::
2018-06-06 03:53:31 :: administrator -> marciana :: 2001
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsAERONOMIA
fotografia todo céu
técnicas de imageamento
metodologia
ionosféricos
bolhas de plasma
deriva de plasma
all sky photography
imaging techniques
methodology
ionospherics
plasma bubbles
plasma drift
AbstractWith the recent advances in all-sky imaging technology for nightglow emission studies, the F-region OI 630 nm emission has become an important tool for ionospheric/thermospheric coupling studies. At equatorial and low latitude regions, the all-sky imaging observations of the OI 630 nm emission show quasi north-south aligned intensity depletion bands, which are the optical signatures of large scale F-region plasma irregularities. By observing the motion of the intensity depleted bands it is possible to infer the ionospheric plasma zonal velocity of the depletion. The north-south aligned structures seen in the field of view of the all-sky imaging system corotate with the ionospheric plasma, so that by calculating the spatial displacements occurring during successive OI 630 nm emission images we can infer the ionospheric plasma drift velocity. However, the plasma bubbles have their own internal space-time dynamics leading to changes in their shape and dimensions and this may induce some errors in the calculated drift velocities. In this paper we take into account the space-time changes in the plasma bubbles in order to calculate the ionospheric plasma zonal drift velocities using the Of 630 nm nightglow emission.
AreaCEA
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4. Conditions of access and use
Target FileIonospheric plasma bubble zonal drift.pdf
User Groupadministrator
jefferson
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
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