Close

1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/36KT6DL
Repositorysid.inpe.br/mtc-m19@80/2009/12.23.15.12   (restricted access)
Last Update2020:11.24.18.54.26 (UTC) seeger5
Metadata Repositorysid.inpe.br/mtc-m19@80/2009/12.23.15.12.02
Metadata Last Update2020:11.24.18.54.26 (UTC) seeger5
Labelself-archiving-INPE-MCTIC-GOV-BR
Citation KeyRigozoEvanNordEche:2009:PrSoMi
TitlePrediction of Solar Minimum and Maximum Epochs on the Basis of Spectral Characteristics for the Next Millennium
Year2009
Access Date2024, May 08
Secondary TypePRE CI
Number of Files1
Size10 KiB
2. Context
Author1 Rigozo, Nivaor Rodolfo
2 Evangelista, H.
3 Nordeman, Daniel Jean Roger
4 Echer, Mariza Pereira de Souza
Group1 CRS-CCR-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference NameInternational Living with a Star, (ILWS/2009).
Conference LocationUbatuba, São Paulo, Brasil
DateOctober, 4-9
History (UTC)2009-12-23 15:12:13 :: seeger5 -> administrator ::
2018-06-05 04:36:08 :: administrator -> seeger5 ::
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsPrediction solar activity
sunspot number time series
Spectral analysis
multiresolution analysis
AbstractA prevision of solar activity minimum and maximum epochs for the next 1000 years was obtained using a sum of sine waves derived from spectral analysis of the time series of 10-years average sunspot number for the period 10162006. The time series was decomposed in frequency levels using the wavelet transform, and an iterative regression model (ARIST) was used to identify the amplitude and phase of the main periodicities. The 1000-year prevision solar activity minimum and maximum epochs seems to represent well the next four minimums and one maximum. The 10-years average sunspot number activity in each anomalous period was used in linear equations to obtain estimates of the solar irradiance, solar wind velocity, and the southward component of the interplanetary magnetic field.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Prediction of Solar...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filerigozo_prediction2.pdf
User Groupseeger5
administrator
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url volume
7. Description control
e-Mail (login)seeger5
update 


Close