Articles | Volume 10, issue 6
https://doi.org/10.5194/gmd-10-2247-2017
https://doi.org/10.5194/gmd-10-2247-2017
Development and technical paper
 | 
22 Jun 2017
Development and technical paper |  | 22 Jun 2017

Solar forcing for CMIP6 (v3.2)

Katja Matthes, Bernd Funke, Monika E. Andersson, Luke Barnard, Jürg Beer, Paul Charbonneau, Mark A. Clilverd, Thierry Dudok de Wit, Margit Haberreiter, Aaron Hendry, Charles H. Jackman, Matthieu Kretzschmar, Tim Kruschke, Markus Kunze, Ulrike Langematz, Daniel R. Marsh, Amanda C. Maycock, Stergios Misios, Craig J. Rodger, Adam A. Scaife, Annika Seppälä, Ming Shangguan, Miriam Sinnhuber, Kleareti Tourpali, Ilya Usoskin, Max van de Kamp, Pekka T. Verronen, and Stefan Versick

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Cited articles

Abreu, J. A., Beer, J., Steinhilber, F., Tobias, S. M., and Weiss, N. O.: For how long will the current grand maximum of solar activity persist?, Geophys. Res. Lett., 35, 20109, https://doi.org/10.1029/2008GL035442, 2008.
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Amblard, P., Moussaoui, S., Dudok de Wit, T., Aboudarham, J., Kretzschmar, M., Lilensten, J., and Auchère, F.: The EUV Sun as the superposition of elementary Suns, Astron. Astrophys., 487, L13–L16, https://doi.org/10.1051/0004-6361:200809588, 2008.
Andersson, M. E., Verronen, P. T., Rodger, C. J., Clilverd, M. A., and Seppälä, A.: Missing driver in the Sun–Earth connection from energetic electron precipitation impacts mesospheric ozone, Nature Commun., 5, 5197, https://doi.org/10.1038/ncomms6197, 2014a.
Andersson, M. E., Verronen, P. T., Rodger, C. J., Clilverd, M. A., and Wang, S.: Longitudinal hotspots in the mesospheric OH variations due to energetic electron precipitation, Atmos. Chem. Phys., 14, 1095–1105, https://doi.org/10.5194/acp-14-1095-2014, 2014b.
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Short summary
The solar forcing dataset for climate model experiments performed for the upcoming IPCC report is described. This dataset provides the radiative and particle input of solar variability on a daily basis from 1850 through to 2300. With this dataset a better representation of natural climate variability with respect to the output of the Sun is provided which provides the most sophisticated and comprehensive respresentation of solar variability that has been used in climate model simulations so far.