data:gases

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data:gases [2019/02/08 11:59] – Added PDGv1-PGMspin and PDGv1 jypeterdata:gases [2019/02/08 14:43] – Added PDGv1-PGMspin and PDGv1 jypeter
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 | LDv1-transpin\\ LDv1 | Transient, as per Loulergue et al. (2008)\\ **Get reference and data below!** | | LDv1-transpin\\ LDv1 | Transient, as per Loulergue et al. (2008)\\ **Get reference and data below!** |
 | PDGv1-PGMspin | 387 | | PDGv1-PGMspin | 387 |
-| PDGv1 | Transient, as per [[#References_cited| the spline of Koehler et al. (2017)]]: [ [[https://doi.pangaea.de/10.1594/PANGAEA.871273|Access to data]] ] |+| PDGv1 | Transient, as per [[exp_design:degla_t2#References_cited| the spline of Koehler et al. (2017)]]: [ [[https://doi.pangaea.de/10.1594/PANGAEA.871273|Access to data]] ] |
  
  
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 | LDv1-transpin\\ LDv1 | Transient, as per Schilt et al. (2010)\\ **Get reference and data below!** | | LDv1-transpin\\ LDv1 | Transient, as per Schilt et al. (2010)\\ **Get reference and data below!** |
 | PDGv1-PGMspin | 201 | | PDGv1-PGMspin | 201 |
-| PDGv1 | Linear increase from 201 ppb at 140 ka to 218.74 ppb at 134.5 ka\\ then transient, as per [[#References_cited| the spline of Koehler et al. (2017)]]: [ [[https://doi.pangaea.de/10.1594/PANGAEA.871273|Access to data]] |+| PDGv1 | Linear increase from 201 ppb at 140 ka to 218.74 ppb at 134.5 ka\\ then transient, as per [[exp_design:degla_t2#References_cited| the spline of Koehler et al. (2017)]]: [ [[https://doi.pangaea.de/10.1594/PANGAEA.871273|Access to data]] ] |
  
  
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 ^ Experiment ^ Value ^ ^ Experiment ^ Value ^
-| midHolocene\\ lgm\\ lig127k\\ midPliocene-eoi400 \\ LDv1-LGMspin\\ LDv1-transpin\\ LDv1 | \\ \\ \\ //Same as in CMIP6 piControl// | +| midHolocene\\ lgm\\ lig127k\\ midPliocene-eoi400 \\ LDv1-LGMspin\\ LDv1-transpin\\ LDv1\\ PDGv1-PGMspin\\ PDGv1 | \\ \\ \\ //Same as in CMIP6 piControl// |
-| PDGv1-PGMspin\\ PDFv1 | Preindustrial (e.g. 10 DU) |+
 | past1000 | For models without interactive ozone chemistry, we suggest that O3 modulation is derived in a similar way from the modulation of the UV part of the solar spectrum as in the historical simulations (c.f. [[http://www.geosci-model-dev-discuss.net/gmd-2016-91/|Matthes et al., CMIP6 GMD special issue 2016]]) | | past1000 | For models without interactive ozone chemistry, we suggest that O3 modulation is derived in a similar way from the modulation of the UV part of the solar spectrum as in the historical simulations (c.f. [[http://www.geosci-model-dev-discuss.net/gmd-2016-91/|Matthes et al., CMIP6 GMD special issue 2016]]) |
  
  • data/gases.txt
  • Last modified: 2019/02/11 11:20
  • by jypeter