Preprints
https://doi.org/10.5194/egusphere-2026-28
https://doi.org/10.5194/egusphere-2026-28
15 Jan 2026
 | 15 Jan 2026
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

Benjamin M. Sanderson, Susanne Baur, Carl-Freidrich Schleussner, Glen P. Peters, Shivika Mittal, Marit Sandstad, Steffen Kallbekken, Chris Smith, Sabine Fuss, Bas van Ruijven, Rosie A. Fisher, Joeri Rogelj, Roland Séférian, Bjørn Samset, Norman J. Steinert, Laurent Terray, and Jan Fuglestvedt

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.

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Benjamin M. Sanderson, Susanne Baur, Carl-Freidrich Schleussner, Glen P. Peters, Shivika Mittal, Marit Sandstad, Steffen Kallbekken, Chris Smith, Sabine Fuss, Bas van Ruijven, Rosie A. Fisher, Joeri Rogelj, Roland Séférian, Bjørn Samset, Norman J. Steinert, Laurent Terray, and Jan Fuglestvedt

Status: open (until 26 Feb 2026)

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Benjamin M. Sanderson, Susanne Baur, Carl-Freidrich Schleussner, Glen P. Peters, Shivika Mittal, Marit Sandstad, Steffen Kallbekken, Chris Smith, Sabine Fuss, Bas van Ruijven, Rosie A. Fisher, Joeri Rogelj, Roland Séférian, Bjørn Samset, Norman J. Steinert, Laurent Terray, and Jan Fuglestvedt
Benjamin M. Sanderson, Susanne Baur, Carl-Freidrich Schleussner, Glen P. Peters, Shivika Mittal, Marit Sandstad, Steffen Kallbekken, Chris Smith, Sabine Fuss, Bas van Ruijven, Rosie A. Fisher, Joeri Rogelj, Roland Séférian, Bjørn Samset, Norman J. Steinert, Laurent Terray, and Jan Fuglestvedt
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Latest update: 15 Jan 2026
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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.
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