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Do Galactic Cosmic Rays Impact the Cirrus Cloud Cover?

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Climate and Weather of the Sun-Earth System (CAWSES)

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Abstract

Atmospheric ions produced through solar-modulated galactic cosmic rays can promote both the nucleation and the growth of aerosols. The potential impact on the cloud cover is subject of current debates. The CAWSES project SAGACITY (SAtellite and model studies of GAlactic cosmic rays and Clouds modulated by solar activITY) focuses on the statistical analysis of this link, using MIPAS-E satellite data. The extinction data, the cloud occurrence frequency, and the cloud index data from MIPAS-E are correlated with the data from the Climax neutron monitor. A superposed epoch analysis of 6 selected Forbush decrease events yields several weak but statistically significant correlations with an excess of positive cloud-GCR correlations. The impact of a 15 % increase in the Climax neutron monitor data is estimated to result in a small decrease in cloud index (corresponding to an increase in cloud opacity) which is most pronounced at 9 km altitude (−9 % to +0.5 %).

Cornelius Schiller is deceased.

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Acknowledgements

This work was funded by the Deutsche Forschungsgemeinschaft under the SPP 1176 (CAWSES) grant SCHI-872/1-1 (SAGACITY). The Climax-Neutron count data are generated within the NSF Grant ATM-0339527 and the MIPAS level 1b and level 2 data are provided by ESA. With great sadness we mourn the death of our dear colleague Cornelius Schiller, who passed away on 3 March 2012.

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Correspondence to Susanne Rohs .

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Rohs, S., Spang, R., Hoffmann, L., Rohrer, F., Schiller, C. (2013). Do Galactic Cosmic Rays Impact the Cirrus Cloud Cover?. In: Lübken, FJ. (eds) Climate and Weather of the Sun-Earth System (CAWSES). Springer Atmospheric Sciences. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-4348-9_5

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