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Explore real-time reconstructions of solar irradiance for space weather applications in the SOTERIA project. Learn about the components and models used to estimate total solar irradiance (TSI) from sunspot and surface image data, as well as ∆14C data. Discover how these reconstructions can contribute to space weather forecasting.
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Real-Time Reconstructions of the Solar Irradiance for Space Weather Applications in the SOTERIA Project Framework L.E.A. Vieira, T. Dudok De Wit, M. Kretzschmar, G. Cessateur Lab. de Physique et Chimie de l'Environnement et de l'Espace CNRS and University of Orleans 7th European Space Weather Week, November 2010
TSI Observations C. Fröhlich
TSI Reconstruction from Surface Images Surface Images (High Cadence) Daily values Semi-empirical model with main assumption: B-field at solar surface causes TSI + SSI variations Components: Spots (contin. images), faculae + network (magnetograms), quiet Sun Model atmospheres 1 free parameter
Filling factors of the five component model • Quiet Sun (q) • Sunspot Umbra (u) • sunspot penumbra (p) • Faculae + Network (f)
SATIRE TSI vs. PMOD composite Wenzler et al. 2006, A&A
TSI Reconstruction from Sunspot Data Surface Images (High Cadence) Daily values
Estimative of the photospheric magnetic flux Krivova et al., A&A, 2007 Vieira & Solanki, A&A, ,2010 Krivova et al., JGR, 2007, Submitted
TSI Reconstruction from ∆14C Daily values Decadal values Solanki et al., 2004
Feedforward network model • Quiet Sun (q) • Sunspot Umbra (u) • sunspot penumbra (p) • Faculae + Network (f)
Real-Time Reconstructions of the Solar Irradiance for Space Weather Applications in the SOTERIA Project Framework L.E.A. Vieira, T. Dudok De Wit, M. Kretzschmar, G. Cessateur Lab. de Physique et Chimie de l'Environnement et de l'Espace CNRS and University of Orleans 7th European Space Weather Week, November 2010