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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/Gwvkp
Repositorysid.inpe.br/iris@1916/2005/06.21.13.37   (restricted access)
Last Update2006:03.02.13.05.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/06.21.13.37.33
Metadata Last Update2018:06.05.01.20.21 (UTC) administrator
Secondary KeyINPE-12621-PRE/7914
ISSN0038-0938
1573-093X
Citation KeyFariaEzRiViNoPr:2004:CoSpCh
TitleA comparison of the spectral characteristics of the Wolf Sunspot Number (R-Z) and Group Sunspot Number (R-G)
Year2004
MonthNov.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size2586 KiB
2. Context
Author1 Faria, Heloisa Helena de
2 Ezequiel, Echer
3 Rigozo, Nivaor Rodolfo
4 Vieira, Luiz Eduardo Antunes
5 Nordemann, Daniel Jean Roger
6 Prestes, Alan
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JGT6
Group1 DGE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial(INPE, LAC)
JournalSolar Physics
Volume223
Number1
Pages305-318
History (UTC)2006-03-02 13:05:29 :: sergio -> administrator ::
2006-09-28 22:27:34 :: administrator -> sergio ::
2008-01-07 12:52:50 :: sergio -> administrator ::
2018-06-05 01:20:21 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSOLAR-ACTIVITY RECONSTRUCTION
MAUNDER MINIMUM
GEOMAGNETIC-ACTIVITY
WAVELET ANALYSIS
WIND VELOCITY
TIME-SERIES
CYCLE
IRRADIANCE
PARAMETERS
MAXIMUM
AbstractThe objective of this paper is to compare the spectral features of the recently derived Group Sunspot Numbers (RG) and the traditional Wolf Sunspot Numbers (RZ) for the 1700-1995 period. In order to study the spectral features of both time series, two methods were used, including: (a) the multitaper analysis and (b) the wavelet analysis. Well-known features of the solar variability, such as the 98.6-yr (Gleissberg cycle), 10-11-yr (Schwabe cycle) and 5-yr (second solar harmonic) periodicities were identified with high confidence using the multitaper analysis. Also observed was a larger amount of power spread in high frequencies for RZ than for RG spectra. Furthermore, a multitaper analysis of two subsets, A (1700-1850) and B (1851-1995), has indicated that the main differences occurred in the first subset and seem to be due to uncertainties in the early observations. The wavelet transform, which allows observing the spectra evolution of both series, showed a strong and persistent 10-11-yr signal that remained during the whole period. The Meyer Wavelet Transform was applied to both RZ and RG. This study indicates that the main spectral characteristics of both series are similar and that their long-term variability has the same behavior.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > A comparison of...
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4. Conditions of access and use
Languageen
Target File100.pdf
User Groupadministrator
sergio
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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