1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZGivnK2Y/QyyyM |
Repository | sid.inpe.br/mtc-m17@80/2007/06.25.17.16 (restricted access) |
Last Update | 2007:06.29.17.30.42 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m17@80/2007/06.25.17.16.01 |
Metadata Last Update | 2021:07.18.04.01.33 (UTC) administrator |
Secondary Key | INPE--PRE/ |
ISSN | 1364-6826 |
Citation Key | Echer:2007:QuOsQB |
Title | On the quasi-biennial oscillation (QBO) signal in the foF2 ionospheric parameter |
Year | 2007 |
Access Date | 2024, Apr. 27 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 221 KiB |
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2. Context | |
Author | Echer, Ezequiel |
Resume Identifier | 8JMKD3MGP5W/3C9JH3D |
Group | DGE-INPE-MCT-BR |
Affiliation | Instituto Nacional de Pesquisas Espaciais (INPE) |
Journal | Journal of Atmospheric and Solar-Terrestrial Physics |
Volume | 69 |
Number | 4-5 |
Pages | 621-627 |
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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Keywords | Solar-terrestrial physics Ionosphere QBO Spectral analysis GEOPHYSICS |
Abstract | The 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > On the quasi-biennial... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | on the quasi biennal.pdf |
User Group | administrator rosemary simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3EU29DP |
Dissemination | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
Host Collection | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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