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Long-Term Changes in the Total Solar Irradiance

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Book cover Motions in the Solar Atmosphere

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 239))

Abstract

During the past two decades, satellite observations have revealed that the total solar irradiance, S⊙, changes both, on the short-time scale (Willson et al., 1981; Willson, 1982) and on the time scale of the solar cycle (Willson et al., 1986). These changes in solar output with magnetic activity could affect the terrestrial climate, especially if larger excursions occurred in the past.

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Authors and Affiliations

  1. Instituto de Astrofisica de Canarias E-38200 La Laguna, Tenerife, Spain

    Manuel Vázquez

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  1. Manuel Vázquez
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  1. Institute of Astronomy, University of Graz, Austria

    Arnold Hanslmeier

  2. Trieste Astronomical Observatory, Italy

    Mauro Messerotti

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© 1999 Springer Science+Business Media Dordrecht

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Vázquez, M. (1999). Long-Term Changes in the Total Solar Irradiance. In: Hanslmeier, A., Messerotti, M. (eds) Motions in the Solar Atmosphere. Astrophysics and Space Science Library, vol 239. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9331-1_7

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  • DOI: https://doi.org/10.1007/978-94-015-9331-1_7

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