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The DeepMIP contribution to PMIP4 : experimental design for model simulations of the EECO, PETM, and pre-PETM (version 1.0)

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Date
23/02/2017
Author
Lunt, Daniel J.
Huber, Matthew
Anagnostou, Eleni
Baatsen, Michiel L. J.
Caballero, Rodrigo
DeConto, Rob
Dijkstra, Henk A.
Donnadieu, Yannick
Evans, David
Feng, Ran
Foster, Gavin L.
Gasson, Ed
Von Der Heydt, Anna S.
Hollis, Chris J.
Inglis, Gordon N.
Jones, Stephen M.
Kiehl, Jeff
Turner, Sandy Kirtland
Korty, Robert L.
Kozdon, Reinhardt
Krishnan, Srinath
Ladant, Jean Baptiste
Langebroek, Petra
Lear, Caroline H.
LeGrande, Allegra N.
Littler, Kate
Markwick, Paul
Otto-Bliesner, Bette
Pearson, Paul
Poulsen, Christopher J.
Salzmann, Ulrich
Shields, Christine
Snell, Kathryn
Stärz, Michael
Super, James
Tabor, Clay
Tierney, Jessica E.
Tourte, Gregory J. L.
Tripati, Aradhna
Upchurch, Garland R.
Wade, Bridget S.
Wing, Scott L.
Winguth, Arne M. E.
Wright, Nicky M.
Zachos, James C.
Zeebe, Richard E.
Keywords
G Geography (General)
GE Environmental Sciences
QA Mathematics
Modelling and Simulation
Earth and Planetary Sciences(all)
DAS
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Abstract
Past warm periods provide an opportunity to evaluate climate models under extreme forcing scenarios, in particular high (> 800ppmv) atmospheric CO2 concentrations. Although a post hoc intercomparison of Eocene (∼ 50 Ma) climate model simulations and geological data has been carried out previously, models of past high-CO2 periods have never been evaluated in a consistent framework. Here, we present an experimental design for climate model simulations of three warm periods within the early Eocene and the latest Paleocene (the EECO, PETM, and pre-PETM). Together with the CMIP6 pre-industrial control and abrupt 4 × CO2 simulations, and additional sensitivity studies, these form the first phase of DeepMIP-the Deep-time Model Intercomparison Project, itself a group within the wider Paleoclimate Modelling Intercomparison Project (PMIP). The experimental design specifies and provides guidance on boundary conditions associated with palaeogeography, greenhouse gases, astronomical configuration, solar constant, land surface processes, and aerosols. Initial conditions, simulation length, and output variables are also specified. Finally, we explain how the geological data sets, which will be used to evaluate the simulations, will be developed.
Citation
Lunt , D J , Huber , M , Anagnostou , E , Baatsen , M L J , Caballero , R , DeConto , R , Dijkstra , H A , Donnadieu , Y , Evans , D , Feng , R , Foster , G L , Gasson , E , Von Der Heydt , A S , Hollis , C J , Inglis , G N , Jones , S M , Kiehl , J , Turner , S K , Korty , R L , Kozdon , R , Krishnan , S , Ladant , J B , Langebroek , P , Lear , C H , LeGrande , A N , Littler , K , Markwick , P , Otto-Bliesner , B , Pearson , P , Poulsen , C J , Salzmann , U , Shields , C , Snell , K , Stärz , M , Super , J , Tabor , C , Tierney , J E , Tourte , G J L , Tripati , A , Upchurch , G R , Wade , B S , Wing , S L , Winguth , A M E , Wright , N M , Zachos , J C & Zeebe , R E 2017 , ' The DeepMIP contribution to PMIP4 : experimental design for model simulations of the EECO, PETM, and pre-PETM (version 1.0) ' , Geoscientific Model Development , vol. 10 , no. 2 , pp. 889-901 . https://doi.org/10.5194/gmd-10-889-2017
Publication
Geoscientific Model Development
Status
Peer reviewed
DOI
https://doi.org/10.5194/gmd-10-889-2017
ISSN
1991-959X
Type
Journal article
Rights
© Author(s) 2017. Published by Copernicus Publications on behalf of the European Geosciences Union. This work is distributed under the Creative Commons Attribution 3.0 License.
Description
We thank NERC grant NE/N006828/1 for providing funds for the first DeepMIP meeting in Boulder, Colorado, USA, in January 2016. Daniel J. Lunt acknowledges the NERC grant “Cretaceous–Paleocene–Eocene: Exploring Climate and Climate Sensitivity” (NE/K014757/1), and advanced ERC grant “The Greenhouse Earth System” (T-GRES, project reference 340923), awarded to Rich Pancost. Matthew Huber acknowledges funding from NSF OCE-0902882. Michiel L. J. Baatsen, Henk A. Dijkstra, and Anna S. von der Heydt acknowledge support by the Netherlands Earth System Science Centre (NESSC), financially supported by the Ministry of Education, Culture and Science (OCW), 024.002.001.
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  • University of St Andrews Research
URI
http://hdl.handle.net/10023/10451

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