https://gmd.copernicus.org/articles/17/2583/2024/

*Authors*
Daniele Visioni, Alan Robock, Jim Haywood, Matthew Henry, Simone Tilmes,
Douglas G. MacMartin, Ben Kravitz, Sarah J. Doherty, John Moore, Chris
Lennard, Shingo Watanabe, Helene Muri, Ulrike Niemeier, Olivier Boucher,
Abu Syed, Temitope S. Egbebiyi, Roland Séférian, and Ilaria Quaglia

*09 April 2024*

https://doi.org/10.5194/gmd-17-2583-2024

*Abstract*
The Geoengineering Model Intercomparison Project (GeoMIP) has proposed
multiple model experiments during phases 5 and 6 of the Climate Model
Intercomparison Project (CMIP), with the latest set of model experiments
proposed in 2015. With phase 7 of CMIP in preparation and with multiple
efforts ongoing to better explore the potential space of outcomes for
different solar radiation modifications (SRMs) both in terms of deployment
strategies and scenarios and in terms of potential impacts, the GeoMIP
community has identified the need to propose and conduct a new experiment
that could serve as a bridge between past iterations and future CMIP7
experiments. Here we report the details of such a proposed experiment,
named G6-1.5K-SAI, to be conducted with the current generation of scenarios
and models from CMIP6 and clarify the reasoning behind many of the new
choices introduced. Namely, compared to the CMIP6 GeoMIP scenario G6sulfur,
we decided on (1) an intermediate emission scenario as a baseline (the
Shared Socioeconomic Pathway 2-4.5), (2) a start date set in the future
that includes both considerations for the likelihood of exceeding 1.5 °C
above preindustrial levels and some considerations for a likely start date
for an SRM implementation, and (3) a deployment strategy for stratospheric
aerosol injection that does not inject in the tropical pipe in order to
obtain a more latitudinally uniform aerosol distribution. We also offer
more details regarding the preferred experiment length and number of
ensemble members and include potential options for second-tier experiments
that some modeling groups might want to run. The specifics of the proposed
experiment will further allow for a more direct comparison between results
obtained from CMIP6 models and those obtained from futu

*Source: EGU*

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