Articles | Volume 21, issue 10
https://doi.org/10.5194/cp-21-1755-2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.Using reduced-complexity volcanic aerosol and climate models to produce large ensemble simulations of Holocene temperature
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- Final revised paper (published on 20 Oct 2025)
- Supplement to the final revised paper
- Preprint (discussion started on 09 Dec 2024)
- Supplement to the preprint
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
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RC1: 'Comment on egusphere-2024-3635', Anonymous Referee #1, 13 Jan 2025
- AC2: 'Reply on RC1', Magali Verkerk, 25 Jun 2025
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RC2: 'Comment on egusphere-2024-3635', Lucie Luecke, 15 May 2025
- AC1: 'Reply on RC2', Magali Verkerk, 25 Jun 2025
Peer review completion
AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Publish subject to minor revisions (review by editor) (07 Jul 2025) by Julien Emile-Geay

AR by Magali Verkerk on behalf of the Authors (09 Jul 2025)
Author's response
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ED: Publish subject to minor revisions (review by editor) (21 Jul 2025) by Julien Emile-Geay

ED: Publish subject to technical corrections (28 Jul 2025) by Julien Emile-Geay

AR by Magali Verkerk on behalf of the Authors (29 Jul 2025)
Manuscript
Comments on: Using reduced-complexity volcanic aerosol and climate models to produce large ensemble simulations of Holocene temperature
Verkerk and coauthors combine reduced-complexity volcanic aerosol (EVA_H) and climate (FaIR) models to simulate the global mean surface temperature (GMST) response to volcanic eruptions over the last 9,000 years (6755 BCE to 1900 CE).
To assess the robustness of their simulations, the authors compare their estimates for the 14 largest eruptions between 1250 CE and 1900 CE with numerous climate reconstructions (Schneider et al., 2015; Wilson et al., 2016; Guillet et al., 2017; Pages2k, 2019; King et al., 2021). The discrepancies between the new simulations and climate reconstructions are notably smaller than in previous studies.
The authors address an important topic. The paper is well-written, well-structured, and easy to follow. The figures are clear and informative. And the authors have made all their simulations publicly available.
The methodology section summarizes well the approach taken by the authors, including the forcing datasets used for the new simulations, the paleo-reconstructions and the climate simulations employed to compare the new results.
Additionally, they acknowledge the limitations of their approach, particularly the Holocene temperature conundrum, which is also apparent in their ensemble simulations of Holocene temperatures.
The authors emphasize the need for future products based on reduced-complexity models to include seasonal and regional outputs, which would be highly valuable for the paleo community.
I appreciated reading the manuscript and, overall, have very few comments to offer. I recommend the paper for acceptance, as I think the new product provided by the authors represents a valuable resource for the paleo community studying past volcanic eruptions. However, I do have one minor suggestion for the authors to consider.
Main text:
Have the authors considered the possibility of comparing the accuracy of their simulations not only against climate/data assimilation reconstructions but also against instrumental datasets, such as the Berkeley Earth Surface Temperature (BEST) dataset? The BEST dataset offers two products that might be of interest: one estimating GMST since 1850 and another providing annual temperature estimates since 1750 (land-only).
Using these datasets could allow the authors to compare their simulations for the 1815 Tambora, 1831 Zavaritskii (Hutchison et al., 2024), and 1883 Krakatau events with “real” temperature observations. Additionally, the Laki eruption might also be investigated, assuming the instrumental records used by BEST are sufficiently dense to represent a reliable global average (which I am not entirely certain about).
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