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Evolution of the solar irradiance during the Holocene

2011/03/25 by Luis Eduardo A. Vieira, L. E. A. Vieira, S. K. Solanki +4 · 3 citations
Biochemistry, Genetics and Molecular Biology · Computer Science · Physics and Astronomy · #Astrophysics #Atmospheric sciences #Geology #Geomagnetism and Paleomagnetism Studies #Geophysics #Heliosphere #Holocene #Irradiance #Magnetic field #Moment (physics) #Oceanography #Optics #Physics #Solar Radiation and Photovoltaics #Solar and Space Plasma Dynamics #Solar irradiance #Solar wind #Sunspot #astro-ph.SR #physics.ao-ph #physics.space-ph

paper · pdf · doi:10.1051/0004-6361/201015843

openalex publication_date 2011/03/25 · arxiv created 2011/03/28 · arxiv updated 2011/05/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. 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.

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