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PMIP4 gases data
CO2
Experiment | Value (ppm) |
---|---|
midHolocene | 264.36 |
lgm | 190 |
past1000 | Time varying Meinshausen et al., CMIP6 GMD special issue |
lig127k | 287 |
midPliocene-eoi400 | 400 |
LDv1-LGMspin | Same as lgm |
LDv1-transpin LDv1 | Transient, as per Bereiter et al. (2015) [ Bereiter et al data access ] |
CH4
Experiment | Value (ppb) |
---|---|
midHolocene | 584.93 |
lgm | 375 |
past1000 | Time varying Meinshausen et al., CMIP6 GMD special issue |
lig127k | 724 |
midPliocene-eoi400 | Same as in CMIP6 piControl |
LDv1-LGMspin | Same as lgm |
LDv1-transpin LDv1 | Transient, as per Loulergue et al. (2008) Get reference and data below! |
Loulergue et al CH4 data
- Reference: Loulergue, L., Schilt, A., Spahni, R., Masson-Delmotte, V., Blunier, T., Lemieux, B., Barnola, J.-M., Raynaud, D., Stocker, T. F. and Chappellaz, J.: Orbital and millennial-scale features of atmospheric CH4 over the past 800,000 years, Nature, 453(7193), 383–386, doi:10.1038/nature06950, 2008.
N20
Experiment | Value (ppb) |
---|---|
midHolocene | 258.56 |
lgm | 200 |
past1000 | Time varying Meinshausen et al., CMIP6 GMD special issue |
lig127k | 262 |
midPliocene-eoi400 | Same as in CMIP6 piControl |
LDv1-LGMspin | Same as lgm |
LDv1-transpin LDv1 | Transient, as per Schilt et al. (2010) Get reference and data below! |
Schilt et al N20 data
- Reference: Schilt, A., Baumgartner, M., Schwander, J., Buiron, D., Capron, E., Chappellaz, J., Loulergue, L., Schüpbach, S., Spahni, R., Fischer, H. and Stocker, T. F.: Atmospheric nitrous oxide during the last 140,000 years, Earth Planet. Sci. Lett., 300(1–2), 33–43, doi:10.1016/j.epsl.2010.09.027, 2010.
CFC
Experiment | Value |
---|---|
midHolocene | 0 |
lgm | 0 |
past1000 | 0 |
lig127k | 0 |
midPliocene-eoi400 | Same as in CMIP6 piControl |
LDv1-LGMspin LDv1-transpin LDv1 | Same as lgm |
O3
Experiment | Value |
---|---|
midHolocene lgm lig127k midPliocene-eoi400 LDv1-LGMspin LDv1-transpin LDv1 | Same as in CMIP6 piControl |
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. Matthes et al., CMIP6 GMD special issue 2016) |