Evolution of solar irradiance during Holocene

DOI

Long-term records of solar radiative output are vital for understanding solar variability and past climate change. Measurements of solar irradiance are available for only the last three decades, which calls for reconstructions of this quantity over longer time scales using suitable models. We present a physically consistent reconstruction of the total solar irradiance for the Holocene.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35310006
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/531/A6
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/531/A6
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/531/A6
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/531/A6
Provenance
Creator Vieira L.E.A.; Solanki S.K.; Krivova N.A.; Usoskin I.
Publisher CDS
Publication Year 2011
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Solar System Astronomy