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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 18, issue 5
Ann. Geophys., 18, 583–588, 2000
https://doi.org/10.1007/s00585-000-0583-z
© European Geosciences Union 2000
Ann. Geophys., 18, 583–588, 2000
https://doi.org/10.1007/s00585-000-0583-z
© European Geosciences Union 2000

  31 May 2000

31 May 2000

Climate hypersensitivity to solar forcing?

W. Soon2,1, E. Posmentier3, and S. Baliunas1 W. Soon et al.
  • 1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA
  • 2Also affiliated with the Faculty of Science and Environmental Studies, University Putra Malaysia, Serdang 43400, Selangor, Malaysia
  • 3Departments of Physics and Mathematics, Long Island University, Brooklyn, New York 11201, USA
  • Correspondence to: W. Soon
  • e-mail: wsoon@cfa.harvard.edu

Abstract. We compare the equilibrium climate responses of a quasi-dynamical energy balance model to radiative forcing by equivalent changes in CO2, solar total irradiance (Stot) and solar UV (SUV). The response is largest in the SUV case, in which the imposed UV radiative forcing is preferentially absorbed in the layer above 250 mb, in contrast to the weak response from global-columnar radiative loading by increases in CO2 or Stot. The hypersensitive response of the climate system to solar UV forcing is caused by strongly coupled feedback involving vertical static stability, tropical thick cirrus ice clouds and stratospheric ozone. This mechanism offers a plausible explanation of the apparent hypersensitivity of climate to solar forcing, as suggested by analyses of recent climatic records. The model hypersensitivity strongly depends on climate parameters, especially cloud radiative properties, but is effective for arguably realistic values of these parameters. The proposed solar forcing mechanism should be further confirmed using other models (e.g., general circulation models) that may better capture radiative and dynamical couplings of the troposphere and stratosphere.

Key words: Meteorology and atmospheric dynamics (climatology · general or miscellaneous) · Solar physics · astrophysics · and astronomy (ultraviolet emissions)

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