Preprints
https://doi.org/10.5194/egusphere-2026-28
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/egusphere-2026-28
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Status: this preprint is open for discussion and under review for Earth System Dynamics (ESD).
Robust assessment of Solar Radiation Modification risks and uncertainties must include shocks and societal feedbacks
Abstract.
Conventional climate scenarios omit fast-timescale human-system dynamics like policy rollback or economic shocks. The climate system's slow response to GHG emissions allows these `fast' terms to be averaged out, a simplification that obscures event-driven risks. Solar Radiation Modification (SRM) invalidates this assumption: rapid, sub-decadal climate responses couple directly to fast political and societal dynamics. This creates an analytical problem: acknowledged primary risks of SRM (termination shock, geopolitical conflict, moral hazard) cannot be resolved in smooth pathways but require an event-based perspective. To address this, we propose the Solar Radiation Modification Pathway (SRMP) framework, introducing five typologies that define governing logic for human-physical system interactions across timescales. We illustrate how SRM-driven shocks could fundamentally divert trajectories from static SSP narratives, revealing limitations in frameworks that assume fixed socio-political contexts. The SRMP framework serves as a diagnostic tool identifying what must be represented for adequate SRM risk assessment. By naming dynamics that current architectures cannot capture, it establishes minimum conditions for assessment that represents the fundamental risks of real-world SRM deployment. If SRM is evaluated primarily through idealised "best-case'' scenarios, the research community risks providing a systematically distorted evidence base for decisions that could prove irreversible.
How to cite. Sanderson, B. M., Baur, S., Schleussner, C.-F., Peters, G. P., Mittal, S., Sandstad, M., Kallbekken, S., Smith, C., Fuss, S., van Ruijven, B., Fisher, R. A., Rogelj, J., Séférian, R., Samset, B., Steinert, N. J., Terray, L., and Fuglestvedt, J.: Robust assessment of Solar Radiation Modification risks and uncertainties must include shocks and societal feedbacks, EGUsphere [preprint], https://doi.org/10.5194/egusphere-2026-28, 2026.
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Status: open (until 26 Feb 2026)
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Benjamin M. Sanderson
CORRESPONDING AUTHOR
CICERO Center for International Climate Change Research, Oslo, Norway
Susanne Baur
Reflective, San Francisco, CA, USA
CNRM, Toulouse, France
Carl-Freidrich Schleussner
International Institute for Applied Systems Analysis, Laxenburg, Austria
Glen P. Peters
CICERO Center for International Climate Change Research, Oslo, Norway
Shivika Mittal
CICERO Center for International Climate Change Research, Oslo, Norway
Marit Sandstad
CICERO Center for International Climate Change Research, Oslo, Norway
Steffen Kallbekken
CICERO Center for International Climate Change Research, Oslo, Norway
Chris Smith
International Institute for Applied Systems Analysis, Laxenburg, Austria
Vrije Universiteit Brussel, Belgium
Sabine Fuss
Potsdam Institute for Climate Impact Research (PIK), Potsdam, Germany
Bas van Ruijven
International Institute for Applied Systems Analysis, Laxenburg, Austria
Rosie A. Fisher
CICERO Center for International Climate Change Research, Oslo, Norway
Joeri Rogelj
International Institute for Applied Systems Analysis, Laxenburg, Austria
Imperial College, London, UK
Roland Séférian
CNRM, Toulouse, France
Bjørn Samset
CICERO Center for International Climate Change Research, Oslo, Norway
Norman J. Steinert
CICERO Center for International Climate Change Research, Oslo, Norway
Laurent Terray
CERFACS, Toulouse, France
Jan Fuglestvedt
CICERO Center for International Climate Change Research, Oslo, Norway
Short summary
Solar Radiation Modification by adding aerosols to the stratosphere could rapidly and temporarily cool the Earth, but this speed creates unprecedented risks. Fast climate responses coupled with political instability create risks of failure to decarbonise, super-rapid climate change, and conflict. Idealized scenarios or conventional modeling tools could lead to systematic ignorance of these risks. We thus introduce a framework outlining what must be represented in future modeling and assessment.
Solar Radiation Modification by adding aerosols to the stratosphere could rapidly and...