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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/marciana/2004/12.03.10.17   (restricted access)
Last Update2004:12.03.02.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/12.03.10.17.50
Metadata Last Update2018:06.05.01.21.09 (UTC) administrator
Secondary KeyINPE-11630-PRE/7011
ISSN0273-1177
Citation KeyBatistaAbdu:2004:CoObIR
TitleIonospheric variability at Brazilian low and equatorial latitudes: comparison between observations and IRI model
Year2004
Access Date2024, May 19
Secondary TypePRE PI
Number of Files1
Size997 KiB
2. Context
Author1 Batista, Inez Staciarini
2 Abdu, Mangalathayil Ali
Resume Identifier1 8JMKD3MGP5W/3C9JHDA
2 8JMKD3MGP5W/3C9JHNK
Group1 DAE-INPE-MCT-BR
JournalAdvances in Space Research
Volume34
Number9
Pages1894-1900
History (UTC)2004-12-14 12:47:49 :: sergio -> administrator ::
2006-09-28 22:27:59 :: administrator -> sergio ::
2008-01-07 12:53:37 :: sergio -> administrator ::
2012-07-17 12:43:27 :: administrator -> marciana ::
2012-10-03 15:59:16 :: marciana -> administrator :: 2004
2018-06-05 01:21:09 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsIonospheric variability
Brazilian low and equatorial latitudes
IRI model
AbstractIonospheric data over two stations in Brazil, one at the magnetic equator and the other close to the southern crest of the equatorial ionization anomaly, during high and low solar activity periods were analyzed. The monthly mean of the parameters foF2 and hmF2 are calculated and compared with the IRI model. The highest discrepancies are observed on post-sunset and nighttime values of foF2 and hmF2 parameters over the equatorial station São Lui´s (2.6°S, 44.2°W, dip angle: -0.5°). In general IRI underestimates hmF2 and overestimates foF2 at the magnetic equatorial station. The effects of post-sunset enhancement of the F-region vertical drift and the resulting intensification of the equatorial ionization anomaly are much stronger in the observation than IRI. The bottomside thickness parameter Bo is also calculated and compared with those used in IRI model.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Ionospheric variability at...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileionospheric variability brazilian.pdf
User Groupadministrator
marciana
sergio
Reader Groupadministrator
marciana
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/bibdigital/2013/09.29.20.43 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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e-Mail (login)marciana
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