https://egusphere.copernicus.org/preprints/2026/egusphere-2026-28/

*Authors: *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

*15 January 2026*

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.

*Source: EGUsphere *

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