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data:gases [2019/02/08 10:59] jypeter Added PDGv1-PGMspin and PDGv1 |
data:gases [2019/02/11 10:20] (current) jypeter Updated the spinup gases |
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| LDv1-LGMspin | //Same as lgm// | | | LDv1-LGMspin | //Same as lgm// | | ||
| LDv1-transpin\\ LDv1 | Transient, as per [[exp_design: | | LDv1-transpin\\ LDv1 | Transient, as per [[exp_design: | ||
- | | PDGv1-PGMspin | 195 | | + | | PDGv1-PGMspin | 191 | |
| PDGv1 | **CO< | | PDGv1 | **CO< | ||
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| LDv1-LGMspin | //Same as lgm// | | | LDv1-LGMspin | //Same as lgm// | | ||
| 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 | 385 | |
- | | PDGv1 | Transient, as per [[# | + | | PDGv1 | Transient, as per [[exp_design: |
Line 46: | Line 46: | ||
| 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 [[# | + | | PDGv1 | Linear increase from 201 ppb at 140 ka to 218.74 ppb at 134.5 ka\\ then transient, as per [[exp_design: |
Line 69: | Line 69: | ||
^ 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:// | | 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:// | ||