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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/QyyyM
Repositorysid.inpe.br/mtc-m17@80/2007/06.25.17.16   (restricted access)
Last Update2007:06.29.17.30.42 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/06.25.17.16.01
Metadata Last Update2021:07.18.04.01.33 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN1364-6826
Citation KeyEcher:2007:QuOsQB
TitleOn the quasi-biennial oscillation (QBO) signal in the foF2 ionospheric parameter
Year2007
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size221 KiB
2. Context
AuthorEcher, Ezequiel
Resume Identifier8JMKD3MGP5W/3C9JH3D
GroupDGE-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume69
Number4-5
Pages621-627
History (UTC)2007-06-29 19:12:19 :: rosemary -> simone ::
2007-12-19 14:22:15 :: simone -> administrator ::
2012-10-23 23:55:01 :: administrator -> simone :: 2007
2013-02-20 15:19:59 :: simone -> administrator :: 2007
2021-07-18 04:01:33 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar-terrestrial physics
Ionosphere
QBO
Spectral analysis
GEOPHYSICS
AbstractThe presence of the quasi-biennial oscillation (QBO) signal in the ionospheric foF2 parameter is investigated using several ionosonde stations. From data continuity, 22 ground-based stations were selected, covering a latitudinal range from 771S to 741N. Monthly average data were filtered using a wavelet multi-resolution method and the data in the band corresponding to the QBO signal (1632 months) were searched with an iterative regression method to find periodicities. Significant periods in that band were found in 13 stations. A QBO-related signal is found in all latitudes and most periods are within 2529 months. The amplitude of QBO is typically 0.150.20 (foF2), which is 10% of the solar cycle signal. Thus the existence of a QBO-type variation in ionosphere was confirmed. Nevertheless, the present analysis does not permit one to conclude if the cause of this variation is related to the solar-geomagnetic QBO, to the stratospheric QBO or to both.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > On the quasi-biennial...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileon the quasi biennal.pdf
User Groupadministrator
rosemary
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
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7. Description control
e-Mail (login)marciana
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