1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m16d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP7W/36KT6DL |
Repository | sid.inpe.br/mtc-m19@80/2009/12.23.15.12 (restricted access) |
Last Update | 2020:11.24.18.54.26 (UTC) seeger5 |
Metadata Repository | sid.inpe.br/mtc-m19@80/2009/12.23.15.12.02 |
Metadata Last Update | 2020:11.24.18.54.26 (UTC) seeger5 |
Label | self-archiving-INPE-MCTIC-GOV-BR |
Citation Key | RigozoEvanNordEche:2009:PrSoMi |
Title | Prediction of Solar Minimum and Maximum Epochs on the Basis of Spectral Characteristics for the Next Millennium |
Year | 2009 |
Access Date | 2024, May 09 |
Secondary Type | PRE CI |
Number of Files | 1 |
Size | 10 KiB |
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2. Context | |
Author | 1 Rigozo, Nivaor Rodolfo 2 Evangelista, H. 3 Nordeman, Daniel Jean Roger 4 Echer, Mariza Pereira de Souza |
Group | 1 CRS-CCR-INPE-MCT-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) |
Conference Name | International Living with a Star, (ILWS/2009). |
Conference Location | Ubatuba, São Paulo, Brasil |
Date | October, 4-9 |
History (UTC) | 2009-12-23 15:12:13 :: seeger5 -> administrator :: 2018-06-05 04:36:08 :: administrator -> seeger5 :: |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | Prediction solar activity sunspot number time series Spectral analysis multiresolution analysis |
Abstract | A 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Prediction of Solar... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | rigozo_prediction2.pdf |
User Group | seeger5 administrator |
Visibility | shown |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53 |
Next Higher Units | 8JMKD3MGPCW/3EUFCFP |
Host Collection | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
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6. Notes | |
Empty Fields | archivingpolicy 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 |
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7. Description control | |
e-Mail (login) | seeger5 |
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