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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/JwH5Q
Repositorysid.inpe.br/iris@1916/2005/12.21.14.22   (restricted access)
Last Update2006:06.16.17.16.19 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/12.21.14.22.13
Metadata Last Update2021:07.18.04.01.21 (UTC) administrator
Secondary KeyINPE-13788--PRE/8974
ISSN1364-6826
Citation KeyPrestesRigoEcheViei:2006:SpAnSu
TitleSpectral analysis of sunspot number and geomagnetic indices 1868-2001
Year2006
MonthJan.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size277 KiB
2. Context
Author1 Prestes, Alan
2 Rigozo, Nivaor Rodolfo
3 Echer, Ezequiel
4 Vieira, Luis Eduardo Antunes
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
Group1 DGE-INPE-MCT-BR
2 DGE-INPE-MCT-BR
3 DGE-INPE-MCT-BR
4 DGE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE, DGE)
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE, DGE)
3 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE, DGE)
4 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE, DGE)
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume68
Number2
Pages182-190
History (UTC)2006-06-16 17:16:19 :: vinicius -> administrator ::
2021-07-18 04:01:21 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordssolar activity
spectral analysis
sunspot number
geomagnetic indices
SOLAR-CYCLE
SEMIANNUAL VARIATION
WIND
AP
OSCILLATIONS
PERIOD
AbstractThe multiple-taper spectral analysis was applied to a(a), A(p) and R-z annual and monthly average series (1868-2001). The significant periods at 95% confidence level for annual averages are 11.1 and 10.2 years for R, and 11.1, 5.3, 4.3, 2.7 and 2.1 years for a(a). For monthly averages, the significant periods were 133 (11.1 years) and 17.7 months for R. and 133 (11.1 years), 63.7 (5.3 years), 17.5, 12.7 and 6 months for aa. The periods associated with the solar cycle are observed in both series. The aa spectrum showed in addition a peak near 4.3 years, which is not present in the R-z spectrum. Other works have also shown this peak in geomagnetic activity. This peak is believed to be caused by the dual-peak structure in the a(a). The 22-year Hale cycle was not detected either in R-z or a(a) spectrum in the period 1868-2001, but it was seen in R-z data for 1700-2000 annual averages. The explanation of this 22-year cycle has been questioned and while in some spectral analysis this periodicity has been found, others have failed in its detection. The aa spectrum showed in addition a peak of 6 months, associated to the semi-annual variation of geomagnetic activity. Three hypotheses have been considered to explain the seasonal activity variation. These are the Russell-McPherron effect, the equinoctial effect and the axial effect.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Spectral analysis of...
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4. Conditions of access and use
Languageen
Target FileSpectral anaysis of sunspot number.pdf
User Groupadministrator
vinicius
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissiontransferred to vinicius
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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