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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/479LM2H
Repositorysid.inpe.br/mtc-m21d/2022/07.15.18.16
Last Update2022:07.15.18.16.07 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/07.15.18.16.07
Metadata Last Update2023:01.03.16.46.10 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyVieiraSilvViei:2022:EvSoLu
TitleEvolution of the solar luminosity science the ende of the maunder minimum
FormatOn-line
Year2022
Access Date2024, May 13
Secondary TypePRE CI
Number of Files1
Size47 KiB
2. Context
Author1 Vieira, Luís Eduardo Antunes
2 Silva, Ligia Alves da
3 Vieira, Icaro
Group1 DIHPA-CGCE-INPE-MCTI-GOV-BR
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Estadual Paulista (UNESP)
Author e-Mail Address1 luis.vieira@inpe.br
2 ligia.alves01@gmail.com
3 icaro.s.viera@gmail.com
Conference NameCOSPAR Scientific Assembly, 44
Conference LocationAthens, Greece
Date16-24 July 2022
History (UTC)2022-07-15 18:16:07 :: simone -> administrator ::
2022-07-16 06:38:20 :: administrator -> simone :: 2022
2022-12-20 12:12:50 :: simone -> administrator :: 2022
2023-01-03 16:46:10 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe total solar irradiance (TSI), the radiant flux at the top of Earths atmosphere and normalized to 1 AU, is part of the solar luminosity in the Earths direction. Reconstructions, which are based on sunspot records since systematic observations, suggest the existence of secular trends in TSI. Although these models correctly incorporate the processes that lead to the variability of the TSI, they make no assumptions regarding the energetics in the convection zone. Here we present a model for the long-term evolution of the solar luminosity based on sunspot observations considering the energy flux in the convection zone. We found that the long-term trend in the solar luminosity (and TSI) is the opposite of the previously suggested by other physics-based models. We discuss in detail our approach and the constraints.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Evolution of the...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 15/07/2022 15:16 1.0 KiB 
4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/479LM2H
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/479LM2H
Languageen
Target FileD2.6-0001-22-oral.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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