This shows you the differences between two versions of the page.
| Both sides previous revision
Previous revision
|
Last revision
Both sides next revision
|
wg:ptof:models [2022/05/18 17:57]
brierley [What model runs might be relevant] |
wg:ptof:models [2022/05/18 17:57]
brierley [What model runs might be relevant] |
| * **[[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://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|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|HadCM3]]** 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]] | * **[[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]] |
| |
| |