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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3P8SECKy/CUaik
Repositorysid.inpe.br/jeferson/2004/07.28.12.35
Last Update2006:06.14.04.09.50 (UTC) administrator
Metadata Repositorysid.inpe.br/jeferson/2004/07.28.12.35.42
Metadata Last Update2018:06.04.04.12.54 (UTC) administrator
Secondary KeyINPE-11071-PRE/6527
ISSN0992-7689
Citation KeyEcherRigoNordViei:2004:PrSoAc
TitlePrediction of solar activity on the basis of spectral characteristics of sunspot number
Year2004
MonthJune
Access Date2024, May 17
Secondary TypePRE PI
Number of Files1
Size280 KiB
2. Context
Author1 Echer, Ezequiel
2 Rigozo, Nivaor Rodolfo
3 Nordemann, Daniel Jean Roger
4 Vieira, Luis Eduardo Antunes
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
2
3 8JMKD3MGP5W/3C9JGT6
Group1 DGE-INPE-MCT-BR
Affiliation1 INPE
2 Faculdade de Tecnologia Thereza Porto Marques (FAETEC)
JournalAnnales Geophysicae
Volume22
Pages2239-2243
History (UTC)2006-09-27 21:00:38 :: administrator -> marciana ::
2008-05-02 16:20:26 :: marciana -> banon ::
2009-07-14 21:35:13 :: banon -> administrator ::
2009-08-12 01:05:32 :: administrator -> banon ::
2010-05-11 15:20:53 :: banon -> administrator ::
2012-10-21 21:46:52 :: administrator -> marciana :: 2004
2013-03-07 14:13:39 :: marciana -> administrator :: 2004
2018-06-04 04:12:54 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsSolar physics
astrophysics and astronomy (instruments and techniques
general or miscellaneous
photosphere and chromosphere)
AbstractPrediction of solar activity strength for solar cycles 23 and 24 is performed on the basis of extrapolation of sunspot number spectral components. Sunspot number data during 1933-1996 periods (solar cycles 17-22) are searched for periodicities by iterative regression. The periods significant at the 95% confidence level were used in a sum of sine series to reconstruct sunspot series, to predict the strength of solar cycles 23 and 24. The maximum peak of solar cycles is adequately predicted (cycle 21: 158±13.2 against an observed peak of 155.4; cycle 22: 178±13.2 against 157.6 observed). Solar cycle 23 was predicted to have a peak in 2000 with maximum amplitude of 125±13.2, in good agreement with the 119.6 observed. The minimum of solar cycle 23 is predicted to occur around 2007-2008. For solar cycle 24, the maximum is predicted to occur in 2012 (115±13.2) or 2013 (117±13.2) and this shall be a very weak solar cycle.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Prediction of solar...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/6qtX3pFwXQZ3P8SECKy/CUaik
zipped data URLhttp://urlib.net/zip/6qtX3pFwXQZ3P8SECKy/CUaik
Languageen
Target Fileag-22-2239.pdf
User Groupadministrator
alexandra
banon
marciana
Visibilityshown
Copy HolderSID/SCD
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 3
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
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7. Description control
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