Status: this preprint is open for discussion and under review for Geoscientific Model Development (GMD).
MioMIP2: Experimental design for Phase 1 & 2 of the Miocene component of the CMIP7/PMIP7 Deep-time Model Intercomparison Project (DeepMIP-Miocene)
Natalie J. Burls,Nicky M. Wright,R. Paul Acosta,Catherine D. Bradshaw,Edward Gasson,Lennert B. Stap,Gilles Ramstein,Anna Ruth W. Halberstadt,Agatha M. De Boer,Funda Akgün,David J. Cantrill,Manuel Casas-Gallego,Nela Doláková,Boglarka Erdei,Alex Farnsworth,Sarah Feakins,Ran Feng,Tamara Fletcher,Frédéric Fluteau,J. A. Mattias Green,Anna S. von der Heydt,Matthew Huber,David K. Hutchinson,Dimiter Ivanov,Mine Sezgül Kayseri-Özer,Gregor Knorr,Marianna Kováčová,Caroline H. Lear,Allegra N. LeGrande,Shufeng Li,Xiaoqing Liu,Daniel J. Lunt,Katrin Meissner,Yunfa Miao,Trusha J. Naik,Javier B. Navarro,Joseph B. Novak,Diana Ochoa,Guy J.G. Paxman,Matthew J. Pound,James W. B. Rae,Tammo Reichgelt,Martin Renoult,Francesca Sangiorgi,Anta-Clarisse Sarr,Diane Segalla,Pierre Sepulchre,Amelia Shevenell,Sebastian Steinig,Eivind Straume,Caroline A. E. Strömberg,Clay Tabor,Torsten Utescher,Julia E. Weiffenbach,Elżbieta Worobiec,Yurui Zhang,Feng Zhu,Jiang Zhu,Alexandra Auderset,Florence Colleoni,Aisling Dolan,Rachel Havranek,Ann Holbourn,Nicholas Herold,Daeun Lee,James W. Marschalek,Bryce Mitsunaga,Sevi Modestou,Lina Perez-Angel,Mae Saslaw,Sinda Sosdian,Elena Stiles,Yong Sun,Ning Tan,Zhongshi Zhang,and Yan Zhao
Abstract. The Miocene Epoch has emerged as an important paleoclimate model intercomparison target due to its dynamic nature, global warmth, and reconstructed atmospheric CO2 concentrations. Miocene CO2 estimates range from as low as 300–600 ppmv to as high as 800–1100 ppmv. The formalized Miocene Model Intercomparison Project (MioMIP2) aims to address questions about the mechanisms driving the climatic changes and tipping points seen in the geological record and improve confidence in the ability of climate models to predict future climates and constrain climate sensitivity. Through alignment with PlioMIP and DeepMIP-Eocene efforts, a coordinated MioMIP (DeepMIP-Miocene) effort will allow for cross-time-period studies that sample the full range of Shared Socioeconomic Pathway paleo analogues. Building on the MioMIP1 “MIP of opportunity”, the Miocene community has been developing the experimental design for MioMIP2. The MioMIP1 effort was an ensemble of opportunity that leveraged existing Miocene simulations run with different models, boundary conditions, and reference datasets. MioMIP2 will be the first formal Miocene MIP with common boundary conditions and will target the Miocene Climatic Optimum (MCO; 16.75–14.5 Ma). We present the experimental design for coordinated “CORE” MCO simulations and sensitivity studies. This community effort synthesizes paleogeography, ice sheet, CO2, and vegetation boundary conditions based on the latest available literature and will use geological data from companion proxy synthesis efforts to evaluate the simulations.
Received: 19 Jun 2026 – Discussion started: 03 Aug 2026
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Natalie J. Burls,Nicky M. Wright,R. Paul Acosta,Catherine D. Bradshaw,Edward Gasson,Lennert B. Stap,Gilles Ramstein,Anna Ruth W. Halberstadt,Agatha M. De Boer,Funda Akgün,David J. Cantrill,Manuel Casas-Gallego,Nela Doláková,Boglarka Erdei,Alex Farnsworth,Sarah Feakins,Ran Feng,Tamara Fletcher,Frédéric Fluteau,J. A. Mattias Green,Anna S. von der Heydt,Matthew Huber,David K. Hutchinson,Dimiter Ivanov,Mine Sezgül Kayseri-Özer,Gregor Knorr,Marianna Kováčová,Caroline H. Lear,Allegra N. LeGrande,Shufeng Li,Xiaoqing Liu,Daniel J. Lunt,Katrin Meissner,Yunfa Miao,Trusha J. Naik,Javier B. Navarro,Joseph B. Novak,Diana Ochoa,Guy J.G. Paxman,Matthew J. Pound,James W. B. Rae,Tammo Reichgelt,Martin Renoult,Francesca Sangiorgi,Anta-Clarisse Sarr,Diane Segalla,Pierre Sepulchre,Amelia Shevenell,Sebastian Steinig,Eivind Straume,Caroline A. E. Strömberg,Clay Tabor,Torsten Utescher,Julia E. Weiffenbach,Elżbieta Worobiec,Yurui Zhang,Feng Zhu,Jiang Zhu,Alexandra Auderset,Florence Colleoni,Aisling Dolan,Rachel Havranek,Ann Holbourn,Nicholas Herold,Daeun Lee,James W. Marschalek,Bryce Mitsunaga,Sevi Modestou,Lina Perez-Angel,Mae Saslaw,Sinda Sosdian,Elena Stiles,Yong Sun,Ning Tan,Zhongshi Zhang,and Yan Zhao
Status: open (until 29 Oct 2026)
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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This manuscript provides a very solid discussion of the MioMIP2 protocol. It gives a nice explanation of the boundary conditions and a justification for them. The updates are described cleanly and the experiments are laid out in a sensible fashion. I would recommend the three points below are addressed prior to publication, and I've also attached an scan with some solely technical corrections (typos etc).
A) The main point that I would like to raise is that, as written, there is a disconnect between the title and the recommendation in my opinion. I feel that you ought to recommend that those modelling groups with a CMIP7-grade model should post their output onto the Earth System Grid Federation. Perhaps you could also give an experiment name for the CMIP controlled vocabulary: at least for the core experiment. Might I suggest miocene-3x? You might also consider rephrasing L220 to make it explicit that groups can directly use their CMIP6/7 piControl, as it currently reads that they might need to rerun it for Deep-MIP. A brief sentence describing how this fits into wider PMIP and CMIP efforts if undertaken with a CMIP7 model would be appreciated.
B) Section 2 seems too short (esp. compared to Sect 3), and more importantly just states the decision to focus on the MCO, rather than justifies it. Perhaps you could fold this into the literature review (stating that you build upon other work that is all focussed on the MCO).
C) I find the evidence you provide in Fig 1 around the CO2 level to be unhelpful. I've no problem with the CO2 levels chosen for the protocol. But I can't see how they relate to the Miocene CO2 estimates shown in Fig 1. Perhaps adding some horizontal lines would help. But I also do not understand the difference between the solid line in Fig 1 and the (much higher) dots.
Natalie J. Burls,Nicky M. Wright,R. Paul Acosta,Catherine D. Bradshaw,Edward Gasson,Lennert B. Stap,Gilles Ramstein,Anna Ruth W. Halberstadt,Agatha M. De Boer,Funda Akgün,David J. Cantrill,Manuel Casas-Gallego,Nela Doláková,Boglarka Erdei,Alex Farnsworth,Sarah Feakins,Ran Feng,Tamara Fletcher,Frédéric Fluteau,J. A. Mattias Green,Anna S. von der Heydt,Matthew Huber,David K. Hutchinson,Dimiter Ivanov,Mine Sezgül Kayseri-Özer,Gregor Knorr,Marianna Kováčová,Caroline H. Lear,Allegra N. LeGrande,Shufeng Li,Xiaoqing Liu,Daniel J. Lunt,Katrin Meissner,Yunfa Miao,Trusha J. Naik,Javier B. Navarro,Joseph B. Novak,Diana Ochoa,Guy J.G. Paxman,Matthew J. Pound,James W. B. Rae,Tammo Reichgelt,Martin Renoult,Francesca Sangiorgi,Anta-Clarisse Sarr,Diane Segalla,Pierre Sepulchre,Amelia Shevenell,Sebastian Steinig,Eivind Straume,Caroline A. E. Strömberg,Clay Tabor,Torsten Utescher,Julia E. Weiffenbach,Elżbieta Worobiec,Yurui Zhang,Feng Zhu,Jiang Zhu,Alexandra Auderset,Florence Colleoni,Aisling Dolan,Rachel Havranek,Ann Holbourn,Nicholas Herold,Daeun Lee,James W. Marschalek,Bryce Mitsunaga,Sevi Modestou,Lina Perez-Angel,Mae Saslaw,Sinda Sosdian,Elena Stiles,Yong Sun,Ning Tan,Zhongshi Zhang,and Yan Zhao
Natalie J. Burls,Nicky M. Wright,R. Paul Acosta,Catherine D. Bradshaw,Edward Gasson,Lennert B. Stap,Gilles Ramstein,Anna Ruth W. Halberstadt,Agatha M. De Boer,Funda Akgün,David J. Cantrill,Manuel Casas-Gallego,Nela Doláková,Boglarka Erdei,Alex Farnsworth,Sarah Feakins,Ran Feng,Tamara Fletcher,Frédéric Fluteau,J. A. Mattias Green,Anna S. von der Heydt,Matthew Huber,David K. Hutchinson,Dimiter Ivanov,Mine Sezgül Kayseri-Özer,Gregor Knorr,Marianna Kováčová,Caroline H. Lear,Allegra N. LeGrande,Shufeng Li,Xiaoqing Liu,Daniel J. Lunt,Katrin Meissner,Yunfa Miao,Trusha J. Naik,Javier B. Navarro,Joseph B. Novak,Diana Ochoa,Guy J.G. Paxman,Matthew J. Pound,James W. B. Rae,Tammo Reichgelt,Martin Renoult,Francesca Sangiorgi,Anta-Clarisse Sarr,Diane Segalla,Pierre Sepulchre,Amelia Shevenell,Sebastian Steinig,Eivind Straume,Caroline A. E. Strömberg,Clay Tabor,Torsten Utescher,Julia E. Weiffenbach,Elżbieta Worobiec,Yurui Zhang,Feng Zhu,Jiang Zhu,Alexandra Auderset,Florence Colleoni,Aisling Dolan,Rachel Havranek,Ann Holbourn,Nicholas Herold,Daeun Lee,James W. Marschalek,Bryce Mitsunaga,Sevi Modestou,Lina Perez-Angel,Mae Saslaw,Sinda Sosdian,Elena Stiles,Yong Sun,Ning Tan,Zhongshi Zhang,and Yan Zhao
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Department of Atmospheric, Oceanic and Earth Sciences & the Center for Ocean-Land-Atmosphere Studies, George Mason University, Fairfax, VA, United States
Department of Atmospheric, Oceanic and Earth Sciences & the Center for Ocean-Land-Atmosphere Studies, George Mason University, Fairfax, VA, United States
Catherine D. Bradshaw
The Global Systems Institute, University of Exeter, Exeter, United Kingdom
Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research, Bremerhaven, Germany
Marianna Kováčová
Department of Geology and Paleontology, Faculty of Natural Sciences, Comenius University Bratislava, Mlynská dolina, Ilkovičova 6, 842 15 Bratislava, Slovak Republic
Climate Change Research Centre, University of New South Wales, Sydney, Australia
Yunfa Miao
Key Laboratory of Ecological Safety and Sustainable Development in Arid Lands, Northwest Institute of Eco-Environment and Resources, Chinese Academy of Sciences, China
State Key Laboratory of Tibetan Plateau Earth System, Resources and Environment (TPESRE), Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing, China
Ning Tan
State Key Laboratory Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
Department of Atmospheric and Oceanic Sciences, School of Physics, School of Earth and Space Science, Peking University, Beijing, China
Yan Zhao
State Key Laboratory of Tibetan Plateau Earth System, Resources and Environment (TPESRE), Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing, China
Simulating warm paleoclimates increases our understanding of the mechanisms that drive climatic change and tipping points. The Miocene Epoch, specifically the Miocene Climatic Optimum, has been identified as a particularly valuable past warm climate to simulate, meriting the design of a coordinated Miocene Model Intercomparison Project. Here we synthesize the latest available literature and present the experimental design for coordinated Miocene simulations and sensitivity studies.
Simulating warm paleoclimates increases our understanding of the mechanisms that drive climatic...
This manuscript provides a very solid discussion of the MioMIP2 protocol. It gives a nice explanation of the boundary conditions and a justification for them. The updates are described cleanly and the experiments are laid out in a sensible fashion. I would recommend the three points below are addressed prior to publication, and I've also attached an scan with some solely technical corrections (typos etc).
A) The main point that I would like to raise is that, as written, there is a disconnect between the title and the recommendation in my opinion. I feel that you ought to recommend that those modelling groups with a CMIP7-grade model should post their output onto the Earth System Grid Federation. Perhaps you could also give an experiment name for the CMIP controlled vocabulary: at least for the core experiment. Might I suggest miocene-3x? You might also consider rephrasing L220 to make it explicit that groups can directly use their CMIP6/7 piControl, as it currently reads that they might need to rerun it for Deep-MIP. A brief sentence describing how this fits into wider PMIP and CMIP efforts if undertaken with a CMIP7 model would be appreciated.
B) Section 2 seems too short (esp. compared to Sect 3), and more importantly just states the decision to focus on the MCO, rather than justifies it. Perhaps you could fold this into the literature review (stating that you build upon other work that is all focussed on the MCO).
C) I find the evidence you provide in Fig 1 around the CO2 level to be unhelpful. I've no problem with the CO2 levels chosen for the protocol. But I can't see how they relate to the Miocene CO2 estimates shown in Fig 1. Perhaps adding some horizontal lines would help. But I also do not understand the difference between the solid line in Fig 1 and the (much higher) dots.