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Eos | Eos Transactions, American Geophysical Union

 

Keywords

  • solar flux
  • cloud physics
  • cosmic ray

Index Terms

  • Global Change: Abrupt/rapid climate change (4901, 8408)
  • Global Change: Climate variability (1635, 3305, 3309, 4215, 4513)
  • Atmospheric Composition and Structure: Cloud physics and chemistry

Abstract

EOS, TRANSACTIONS AMERICAN GEOPHYSICAL UNION, VOL. 90, NO. 44, PAGE 397, 2009
doi:10.1029/2009EO440001

FEATURE

The Terrestrial Cosmic Ray Flux: Its Importance for Climate

Michael Ram

Department of Physics, State University of New York at Buffalo

Michael R. Stolz

Department of Physics, State University of New York at Buffalo

Brian A. Tinsley

Department of Physics and Center for Space Sciences, University of Texas at Dallas

There has been prolonged debate in the scientific community as to whether or not changes in solar activity significantly affect Earth's climate. One of the main arguments against solar influence is that because the intensity of solar radiation changes by too little (˜0.1%) during the course of a solar cycle (or on longer time scales) to have a significant impact on changes in Earth's climate, an amplifying mechanism must be at work if solar influence is to be taken seriously. Ney [1959] proposed that the solar-modulated terrestrial cosmic ray flux (CRF) is another solar influence that must be considered as possibly affecting climate. The CRF affects the electrical conductivity of the atmosphere through ion production and is the meteorological variable subject to the largest solar cycle modulation that penetrates into the denser layers of the atmosphere.

Citation: Ram, M., M. R. Stolz, and B. A. Tinsley (2009), The Terrestrial Cosmic Ray Flux: Its Importance for Climate, Eos Trans. AGU, 90(44), 397, doi:10.1029/2009EO440001.

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