Preprints
https://doi.org/10.5194/egusphere-2026-4200
https://doi.org/10.5194/egusphere-2026-4200
31 Jul 2026
 | 31 Jul 2026
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Understanding drivers of inter-model uncertainty in the dynamical response to stratospheric heating

Colleen Marie Golja, Marianna Linz, Ewa Monika Bednarz, Daniele Visioni, Ben Kravitz, John A. Dykema, Michelle E. Frazer, Anthony C. Jones, Isla R. Simpson, and Shingo Watanabe

Abstract. Stratospheric aerosol injection has emerged as a candidate climate intervention strategy to partially offset global surface warming. Previous work has demonstrated that lower stratospheric heating drives modifications to the stratospheric thermal profile, circulation, and water vapor, with downstream consequences for surface climate; however, the impact of stratospheric heating has not previously been characterized across a multi-model ensemble. This work presents first results from the Stratospheric Heating Model Intercomparison Project (SHeatMIP), in which an idealized 0.3 K/day tropical lower-stratospheric heating tendency is imposed across five climate models (CESM, GFDL, GISS, MIROC, UKESM). All models show robust increases in lower-stratospheric temperature, water vapor, and polar night jet strength in both hemispheres, with corresponding surface shifts in the subtropical and eddy-driven jets and a polar cap pressure response resembling a positive North Atlantic Oscillation phase. Despite qualitative agreement, inter-model spread is substantial, with differences of 1 K in the cold point temperature adjustment and 0.38 K in the global mean surface temperature response. The surface temperature spread strongly co-varies with the stratospheric water vapor response (R2 = 0.82), implicating water vapor as a key source of surface warming uncertainty. The forced polar vortex response shows strong co-variability with the climatological polar night jet strength (R2=0.98), and projects onto the surface as a polar cap pressure anomaly. The results show that inter-model differences in the response to stratospheric heating may be traceable to the climatological mean state, offering a pathway toward observationally-constrained evaluation of model suitability for SAI research.

Competing interests: At least one of the (co-)authors is a member of the editorial board of Atmospheric Chemistry and Physics.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Colleen Marie Golja, Marianna Linz, Ewa Monika Bednarz, Daniele Visioni, Ben Kravitz, John A. Dykema, Michelle E. Frazer, Anthony C. Jones, Isla R. Simpson, and Shingo Watanabe

Status: open (until 11 Sep 2026)

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Colleen Marie Golja, Marianna Linz, Ewa Monika Bednarz, Daniele Visioni, Ben Kravitz, John A. Dykema, Michelle E. Frazer, Anthony C. Jones, Isla R. Simpson, and Shingo Watanabe

Data sets

Replication Data for : Understanding drivers of inter-model uncertainty in the dynamical response to stratospheric heating (Version 1) Colleen Golja https://doi.org/10.5281/zenodo.21345483

Colleen Marie Golja, Marianna Linz, Ewa Monika Bednarz, Daniele Visioni, Ben Kravitz, John A. Dykema, Michelle E. Frazer, Anthony C. Jones, Isla R. Simpson, and Shingo Watanabe
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Latest update: 31 Jul 2026
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Short summary
Adding reflective particles to the stratosphere has been proposed to cool the planet, but how the resulting lower-stratospheric heating affects the broader climate remains unclear. This study simulates idealized lower-stratospheric heating across five climate models finding large inter-model differences in the stratospheric and surface response. The results highlight ways in which these differences may be explained by biases in the stratospheric climatological mean state.
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