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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/Sverh
Repositorysid.inpe.br/mtc-m17@80/2007/12.19.13.52   (restricted access)
Last Update2007:12.19.13.52.34 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/12.19.13.52.35
Metadata Last Update2018:06.05.03.36.45 (UTC) administrator
Secondary KeyINPE-15105-PRE/10012
DOI10.1007/s11207-007-9050-2
ISSN0038-0938
1573-093X
Citation KeyKane:2007:SoCyPr
TitleSolar Cycle Predictions based on Solar Activity at Different Solar Latitudes
Year2007
MonthDec.
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size359 KiB
2. Context
AuthorKane, Rajaram Purushottam
Resume Identifier8JMKD3MGP5W/3C9JJ4U
GroupDGE-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
JournalSolar Physics
Volume246
Number2
Pages471-485
History (UTC)2007-12-19 13:52:35 :: simone -> administrator ::
2012-11-17 02:52:25 :: administrator -> simone :: 2007
2013-02-20 15:20:16 :: simone -> administrator :: 2007
2018-06-05 03:36:45 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar cycle - Sunspots - Predictions
AbstractMany methods of predictions of sunspot maximum number use data before or at the preceding sunspot minimum to correlate with the following sunspot maximum of the same cycle, which occurs a few years later. Kane and Trivedi (Solar Phys. 68, 135, 1980) found that correlations of R z(max) (the maximum in the 12-month running means of sunspot number R z) with R z(min) (the minimum in the 12-month running means of sunspot number R z) in the solar latitude belt 20°  40°, particularly in the southern hemisphere, exceeded 0.6 and was still higher (0.86) for the narrower belt > 30° S. Recently, Javaraiah (Mon. Not. Roy. Astron. Soc. 377, L34, 2007) studied the relationship of sunspot areas at different solar latitudes and reported correlations 0.95  0.97 between minima and maxima of sunspot areas at low latitudes and sunspot maxima of the next cycle, and predictions could be made with an antecedence of more than 11 years. For the present study, we selected another parameter, namely, SGN, the sunspot group number (irrespective of their areas) and found that SGN(min) during a sunspot minimum year at latitudes > 30° S had a correlation +0.78±0.11 with the sunspot number R z(max) of the same cycle. Also, the SGN during a sunspot minimum year in the latitude belt (10°  30° N) had a correlation +0.87±0.07 with the sunspot number R z(max) of the next cycle. We obtain an appropriate regression equation, from which our prediction for the coming cycle 24 is R z(max )=129.7±16.3.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Solar Cycle Predictions...
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4. Conditions of access and use
Languageen
Target Filesolar cycle predictions.pdf
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simone
Visibilityshown
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Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES.
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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