Galactic Cosmic Rays - GFZ

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Yu et al. (2008: ACP)Aerosol Nucleation due to <strong>Cosmic</strong>• Maximum influenceon aerosol formationin the upper tropicaltroposphere (10 – 15km) height• Subsequent influenceon clouds not known<strong>Rays</strong>
• Calculations in a climate model with advanced aerosol physics’on-line’• Explicitly calculate the effect of ionization on aerosolnucleation• Focus on changes over a solar cycle
Page 1 and 2: Nacreous clouds over Oslo Source:Ae
Page 3: Correlations betweenGalactic Cosmic
Page 6 and 7: Suggested Mechanisms• Absorption
Page 8 and 9: GCR Ion Production vs. HeightSolar
Page 10 and 11: Forbush Decrease Events
Page 12 and 13: Kristjánsson et al. (2008: ACP)Reg
Page 16: Signals of cosmic rays in particle
Page 19: Signals in SW or LW Radiation atTOA
Page 23: Net Cloud Forcing• Following an F
Page 26 and 27: Correlations between cosmic raysand
Page 29 and 30: Aerosol NucleationMeasurementsKulma
Page 31 and 32: Will the CERN experiments bring new
Page 36 and 37: Pierce & Adams (2009: Geophys.Res.L
Page 38 and 39: Rising Temperatures - No Trend in C
Page 40 and 41: Foto: Michael GaussThank you!http:/
Page 42 and 43: How relevant are Svensmark’sfindi
Page 45 and 46: Ionization distribution• Calculat
Page 47 and 48: GCR, TSI and Low CloudsKristjánsso
Page 49 and 50: Foukal et al. (2004: Science)Blue c
Page 51 and 52: Pre-historic climate variations and
Page 53 and 54: Is the signal really coming from lo

Galactic Cosmic Rays - GFZ

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