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AGU: Geophysical Research Letters

 

Keywords

  • Forbush decrease
  • aerosols
  • clouds

Index Terms

  • Planetary Sciences: Solid Surface Planets: Atmospheres
  • Space Plasma Physics: Ionization processes
  • Solar Physics, Astrophysics, and Astronomy: Coronal mass ejections

Abstract

Cosmic ray decreases affect atmospheric aerosols and clouds

Henrik Svensmark

National Space Institute, Technical University of Denmark, Copenhagen, Denmark

Torsten Bondo

National Space Institute, Technical University of Denmark, Copenhagen, Denmark

Jacob Svensmark

National Space Institute, Technical University of Denmark, Copenhagen, Denmark

Close passages of coronal mass ejections from the sun are signaled at the Earth's surface by Forbush decreases in cosmic ray counts. We find that low clouds contain less liquid water following Forbush decreases, and for the most influential events the liquid water in the oceanic atmosphere can diminish by as much as 7%. Cloud water content as gauged by the Special Sensor Microwave/Imager (SSM/I) reaches a minimum ≈7 days after the Forbush minimum in cosmic rays, and so does the fraction of low clouds seen by the Moderate Resolution Imaging Spectroradiometer (MODIS) and in the International Satellite Cloud Climate Project (ISCCP). Parallel observations by the aerosol robotic network AERONET reveal falls in the relative abundance of fine aerosol particles which, in normal circumstances, could have evolved into cloud condensation nuclei. Thus a link between the sun, cosmic rays, aerosols, and liquid-water clouds appears to exist on a global scale.

Received 31 March 2009; accepted 17 June 2009; published 1 August 2009.

Citation: Svensmark, H., T. Bondo, and J. Svensmark (2009), Cosmic ray decreases affect atmospheric aerosols and clouds, Geophys. Res. Lett., 36, L15101, doi:10.1029/2009GL038429.

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