Articles | Volume 18, issue 24
https://doi.org/10.5194/gmd-18-10095-2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
An emulator-based modelling framework for studying astronomical controls on ocean anoxia with an application to the Devonian
Download
- Final revised paper (published on 18 Dec 2025)
- Supplement to the final revised paper
- Preprint (discussion started on 02 Jun 2025)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
- RC1: 'Comment on egusphere-2025-1696', Anonymous Referee #1, 23 Jul 2025
- RC2: 'Comment on egusphere-2025-1696', Anonymous Referee #2, 07 Aug 2025
- AC1: 'Comment on egusphere-2025-1696', Loïc Sablon, 07 Sep 2025
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Loïc Sablon on behalf of the Authors (02 Oct 2025)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (26 Nov 2025) by Paul Halloran
AR by Loïc Sablon on behalf of the Authors (02 Dec 2025)
Manuscript
Post-review adjustments
AA – Author's adjustment | EA – Editor approval
AA by Loïc Sablon on behalf of the Authors (12 Dec 2025)
Author's adjustment
Manuscript
EA: Adjustments approved (15 Dec 2025) by Paul Halloran
Summary and general review
In the manuscript ‘An Emulator-Based Modelling Framework for Studying Astronomical Controls on Ocean Anoxia with an Application on the Devonian’, Sablon and co-authors couple an emulator to GEOCLIM to evaluate the role of orbital forcing on climate fields and it influence on weathering and nutrient dynamics. The first part of the manuscript outlines the method to build and test the Devonian climate emulator in detail. Their emulator predicts the temperature and runoff fields under a range of orbital parameters and pCO2 with good accuracy. In the second part, the climate emulator is coupled to GEOCLIM to simulate how orbitally driven climate changes affect regolith build-up and weathering in a Devonian configuration. They find that regolith grows during high eccentricity (wetter conditions increase regolith production more than erosion) but the impact on nutrient fluxes is small.
Overall, the manuscript is well structured with the aims and objectives clearly defined. It makes two significant scientific contributions. First, by creating a Devonian climate emulator capable of emulating climate under different CO2 and orbits that demonstrates the sensitivity of Devonian climate to these input parameters. This in itself is an incredibly valuable outcome. Second, the emulator coupled GEOCLIM is the first model that can test hypotheses for recurring Devonian OAEs in a transient manner on multi-Myr timescales. The authors have succeeded in clearly outlining the multi-step approach to build the emulator and add on to the GEOCLIM framework, making it suitable for publication in GMD. However, a few points outlined in the attached document (primarily asking to clarification) should be addressed.