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wg:ptof:models [2021/08/21 10:50] jypeter Removed the discussion after the page got some spam |
wg:ptof:models [2022/10/03 14:39] brierley |
* **Other Transient Simulations** //There are several other long palaeoclimate simulations that my be useful// | * **Other Transient Simulations** //There are several other long palaeoclimate simulations that my be useful// |
* **[[https://www.earthsystemgrid.org/project/trace.html|TraCE]]** This simulation runs from 22,000 years before present (22ka) to 1990 CE as well as single-forcing sensitivity simulations of varying lengths. Contact [[mailto:ottobli@ucar.edu|Bette Otto-Bliesner]] | * **[[https://www.earthsystemgrid.org/project/trace.html|TraCE]]** This simulation runs from 22,000 years before present (22ka) to 1990 CE as well as single-forcing sensitivity simulations of varying lengths. Contact [[mailto:ottobli@ucar.edu|Bette Otto-Bliesner]] |
| * **[[https://www.cesm.ucar.edu/experiments/cesm1.3/iTRACE/|iTraCE]]** This simulation runs from 22,000 years before present (22ka) to around 11ka as well as single-forcing sensitivity simulations of varying lengths. It also includes isotopes. Contact [[mailto:ottobli@ucar.edu|Bette Otto-Bliesner]] |
* **[[https://www.clim-past-discuss.net/cp-2018-140/|MPI]]** Simulations with both fast and slow forcings from 8000ka-present. Contact [[mailto:johann.jungclaus@mpimet.mpg.de|Johann Jungclaus]]. | * **[[https://www.clim-past-discuss.net/cp-2018-140/|MPI]]** Simulations with both fast and slow forcings from 8000ka-present. Contact [[mailto:johann.jungclaus@mpimet.mpg.de|Johann Jungclaus]]. |
* **[[https://doi.org/10.1029/2018GL079337|Kiel]]** Simulations of both the Holocene and the Eemian exist for the Kiel model. Contact [[mailto:vyacheslav.khon@ifg.uni-kiel.de|Vyacheslav Khon]]. | * **[[https://doi.org/10.1029/2018GL079337|Kiel]]** Simulations of both the Holocene and the Eemian exist for the Kiel model. Contact [[mailto:vyacheslav.khon@ifg.uni-kiel.de|Vyacheslav Khon]]. |
* **[[https://www.palmod.de/home|AWI]]** Slowly a simulation from the Last Glacial to present is being is created. Contact [[mailto:Gerrit.Lohmann@awi.de|Gerrit Lohmann]] | * **[[https://www.palmod.de/home|AWI]]** Slowly a simulation from the Last Glacial to present is being is created. Contact [[mailto:Gerrit.Lohmann@awi.de|Gerrit Lohmann]] |
* **[[https://www.clim-past-discuss.net/cp-2018-140/|IPSL]]** Several simulations from 6000ka to present have recently been performed in France. Contact [[mailto:pascale.braconnot@lsce.ipsl.fr|Pascale Braconnot]] and Olivier Marti. | * **[[https://www.clim-past-discuss.net/cp-2018-140/|IPSL]]** Several simulations from 6000ka to present have recently been performed in France. Contact [[mailto:pascale.braconnot@lsce.ipsl.fr|Pascale Braconnot]] and Olivier Marti. |
* **[[https://link.springer.com/article/10.1007/s00382-011-1283-y|FAMOUS]]** A simulation of the last glacial cycle with accelerated-forcing. Contact [[mailto:r.s.smith@reading.ac.uk|Robin Smith]] | * **[[https://link.springer.com/article/10.1007/s00382-011-1283-y|FAMOUS]]** An old simulation of the last glacial cycle with accelerated-forcing. Contact [[mailto:r.s.smith@reading.ac.uk|Robin Smith]] |
* **[[https://www.paleo.bristol.ac.uk/ummodel/scripts/papers/Singarayer_and_Valdes_2010.html|HadCM3]]** There are a series of equilibrium simulations of HadCM3 run over the last glacial cycle. A version of these does exist with water isotopes. Contact [[mailto:j.s.singarayer@reading.ac.uk|Joy Singarayer]] | * **[[https://www.su.se/english/profiles/qzhan-1.191706|EC-Earth3]]** Simulation from about 8ka. Contact [[mailto:qiong.zhang@natgeo.su.se|Qiong Zhang]] |
| * **[[https://gmd.copernicus.org/preprints/gmd-2022-49/|CESM1.2.1]]** Simulation from 11.7 onwards. Contact Zhiping Tian and [[mailto:jiangdb@mail.iap.ac.cn|Dabang Jiang]] |
| * **[[https://www.paleo.bristol.ac.uk/ummodel/scripts/papers/Singarayer_and_Valdes_2010.html|HadCM3]]** A set of transient sensitivity simulations since the deglacial. There are also series of equilibrium simulations of HadCM3 run over the last glacial cycle. A version of these does exist with water isotopes. Contact [[mailto:P.J.Valdes@bristol.ac.uk|Paul Valdes]] |
| * **[[https://www.paleo.bristol.ac.uk/ummodel/scripts/papers/Singarayer_and_Valdes_2010.html|GISS]]** There are a series of equilibrium simulations of GISS-E2-1-G run during the Holocene, potentially with water isotopes. Contact [[mailto:al2035@columbia.edu|Allegra LeGrande]] |
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======= PMIP4/CMIP6 Information ======= | ======= PMIP4/CMIP6 Information ======= |