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Geoscientific Model Development An interactive open-access journal of the European Geosciences Union
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Volume 10, issue 6
Geosci. Model Dev., 10, 2247–2302, 2017
https://doi.org/10.5194/gmd-10-2247-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue: Coupled Model Intercomparison Project Phase 6 (CMIP6) Experimental...

Geosci. Model Dev., 10, 2247–2302, 2017
https://doi.org/10.5194/gmd-10-2247-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.

Development and technical paper 22 Jun 2017

Development and technical paper | 22 Jun 2017

Solar forcing for CMIP6 (v3.2)

Katja Matthes et al.

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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.
Alley, R. B., Berntsen, T., and Bindoff, N. L.: Climate Change 2007 – The Physical Science Basis. Working Group I Contribution to the Fourth Assessment Report of the IPCC, Cambridge University Press, Cambridge, 2007.
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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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.
The solar forcing dataset for climate model experiments performed for the upcoming IPCC report...
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