wg:ptof:models

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
wg:ptof:models [2019/05/21 08:34]
brierley [What model runs might be relevant]
wg:ptof:models [2022/10/03 14:39] (current)
brierley
Line 1: Line 1:
 /* Allow comments in a discussion section at the bottom of the page /* Allow comments in a discussion section at the bottom of the page
-More details: https://www.dokuwiki.org/plugin:discussion */+More details: https://www.dokuwiki.org/plugin:discussion
 ~~DISCUSSION~~ ~~DISCUSSION~~
 Contact  --- //[[jules@blueskiesresearch.org.uk|Julia Hargreaves]] // to contribute to this page, or leave a comment in the discussion box. Contact  --- //[[jules@blueskiesresearch.org.uk|Julia Hargreaves]] // to contribute to this page, or leave a comment in the discussion box.
 + */
  
 /* This is a comment /* This is a comment
Line 57: Line 58:
   * **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]]** 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 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]]   
  
 ======= PMIP4/CMIP6 Information ======= ======= PMIP4/CMIP6 Information =======
  • wg/ptof/models.1558427699.txt.gz
  • Last modified: 2019/05/21 08:34
  • by brierley