Table of Contents

PMIP4 gases data

CO2

Experiment Value (ppm)
midHolocene 264.4
lgm 190
past1000 Time varying
Meinshausen et al., CMIP6 GMD special issue
lig127k 275
midPliocene-eoi400 400
LDv1-LGMspin Same as lgm
LDv1-transpin
LDv1
Transient, as per Bereiter et al. (2015)
[ Bereiter et al data access ] (md5sum = c54a033d8cbf588bc2b95d3b92ff9b1c)
PDGv1-PGMspin 191
PDGv1 CO2 = Transient, as per the spline of Koehler et al. (2017): [ Access to data ]

CH4

Experiment Value (ppb)
midHolocene 597
lgm 375
past1000 Time varying
Meinshausen et al., CMIP6 GMD special issue
lig127k 685
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!
PDGv1-PGMspin 385
PDGv1 Transient, as per the spline of Koehler et al. (2017): [ Access to data ]

Loulergue et al CH4 data

N20

Experiment Value (ppb)
midHolocene 262
lgm 200
past1000 Time varying
Meinshausen et al., CMIP6 GMD special issue
lig127k 255
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!
PDGv1-PGMspin 201
PDGv1 Linear increase from 201 ppb at 140 ka to 218.74 ppb at 134.5 ka
then transient, as per the spline of Koehler et al. (2017): [ Access to data ]

Schilt et al N20 data

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
PDGv1-PGMspin
PDGv1
0

O3

Experiment Value
midHolocene
lgm
lig127k
midPliocene-eoi400
LDv1-LGMspin
LDv1-transpin
LDv1
PDGv1-PGMspin
PDGv1



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)