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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/Hocth
Repositorysid.inpe.br/iris@1916/2005/09.06.12.39   (restricted access)
Last Update2005:09.06.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/09.06.12.39.41
Metadata Last Update2018:06.05.01.16.08 (UTC) administrator
Secondary KeyINPE-13056-PRE/8323
ISSN0038-0938
1573-093X
Citation KeyKane:2005:ShPeSo
TitleShort-term periodicities in solar indices
Year2005
MonthMar.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size4777 KiB
2. Context
AuthorKane, Rajaram Purushottam
Resume Identifier8JMKD3MGP5W/3C9JJ4U
GroupDGE-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial (INPE, DGE)
JournalSolar Physics
Volume227
Number1
Pages155-175
History (UTC)2005-09-06 12:39:41 :: sergio -> administrator ::
2006-09-28 22:30:14 :: administrator -> sergio ::
2008-01-07 12:52:56 :: sergio -> administrator ::
2008-06-10 22:39:44 :: administrator -> marciana ::
2011-05-22 03:44:57 :: marciana -> administrator ::
2018-06-05 01:16:08 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsENTROPY SPECTRAL-ANALYSIS
QUASI-BIENNIAL OSCILLATIONS
COSMIC-RAY INTENSITY
OPEN MAGNETIC-FLUX
ARTIFICIAL SAMPLES
CYCLE
IRRADIANCE
PARAMETERS
FIELD
AbstractThe purpose of the present communication is to identify the short-term ( fewtens of months) periodicities of several solar indices ( sunspot number, CaII area and K index, Lyman a, 2800 MHz radio emission, coronal green-line index, solar magnetic field). The procedure used was: from the 3-month running means (3m) the 37-month running means (37m) were subtracted, and the factor (3m-37m) was examined for several parameters. For solar indices, considerable fluctuations were seen during the +/- 4 years around sunspot maxima of cycles 18- 23, and virtually no fluctuations were seen in the +/- 2 years around sunspot minima. The spacings between successive peaks were irregular but common for various solar indices. Assuming that there are stationary periodicities, a spectral analysis was carried out which indicated periodicities of months: 5.1 - 5.7, 6.2 - 7.0, 7.6 - 7.9, 8.9 - 9.6, 10.4 - 12.0, 12.8 - 13.4, 14.5 - 17.5, 22 - 25, 28 (QBO), 31 - 36 ( QBO), 41 - 47 (QTO). The periodicities of 1.3 year ( 15.6 months) and 1.7 years (20.4 months) often mentioned in the literature were seen neither often nor prominently. Other periodicities occurred more often and more prominently. For the open magnetic flux estimated by Wang, Lean, and Sheeley ( 2000) and Wang and Sheeley ( 2002), it was noticed that the variations were radically different at different solar latitudes. The open flux for <45&DEG; solar latitudes had variations very similar ( parallel) to the sunspot cycle, while open flux for > 45&DEG; solar latitudes had variations anti-parallel to the sunspot cycle. The open fluxes, interplanetary magnetic field and cosmic rays, all showed periodicities similar to those of solar indices. Many peaks ( but not all) matched, indicating that the open flux for < 45&DEG; solar latitudes was at least partially an adequate carrier of the solar characteristics to the interplanetary space and thence for galactic cosmic ray modulation. .
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Short-term periodicities in...
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4. Conditions of access and use
Languageen
Target Fileshort-term.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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