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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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Volume 9, issue 22
Atmos. Chem. Phys., 9, 9043–9057, 2009
https://doi.org/10.5194/acp-9-9043-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.
Atmos. Chem. Phys., 9, 9043–9057, 2009
https://doi.org/10.5194/acp-9-9043-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.

  30 Nov 2009

30 Nov 2009

Initial fate of fine ash and sulfur from large volcanic eruptions

U. Niemeier1, C. Timmreck1, H.-F. Graf2, S. Kinne1, S. Rast1, and S. Self3 U. Niemeier et al.
  • 1Max Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, Germany
  • 2University of Cambridge, Centre for Atmospheric Science, Downing Place, Cambridge, CB2 3EN, UK
  • 3Department of Earth Science, Open University, Milton Keynes, MK7 6AA, UK

Abstract. Large volcanic eruptions emit huge amounts of sulfur and fine ash into the stratosphere. These products cause an impact on radiative processes, temperature and wind patterns. In simulations with a General Circulation Model including detailed aerosol microphysics, the relation between the impact of sulfur and fine ash is determined for different eruption strengths and locations, one in the tropics and one in high Northern latitudes. Fine ash with effective radii between 1 μm and 15 μm has a lifetime of several days only. Nevertheless, the strong absorption of shortwave and long-wave radiation causes additional heating and cooling of ±20 K/day and impacts the evolution of the volcanic cloud. Depending on the location of the volcanic eruption, transport direction changes due to the presence of fine ash, vortices develop and temperature anomalies at ground increase. The results show substantial impact on the local scale but only minor impact on the evolution of sulfate in the stratosphere in the month after the simulated eruptions.

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