h. shiogama 1, m. watanabe 2, t ogura 1, m. yoshiomori 2, t yokohata 1, j.d. annan 3, j.c....
TRANSCRIPT
H. Shiogama1, M. Watanabe2, T Ogura1, M. Yoshiomori2, T Yokohata1, J.D. Annan3, J.C. Hargreaves3, M. Abe1, S. Emori 1, T. Nozawa1, A. Abe-Ouchi2, and M. Kimoto2
1National Institute for Environmental Studies, Tsukuba, Japan 2Atmosphere and Ocean Research Institute, The University of Tokyo, Kashiwa, Japan
3Japan Agency for Marine-Earth Science and Technology,Shinsugita, Japan
To investigate physics parameter uncertainty of climate sensitivity (CS), we are performing a new physics parameter ensemble (PPE) of the MIROC5 coupled atmosphere-ocean general circulation model (CGCM). Previous studies of PPE have mainly used atmosphere-slab ocean model (ASGCM). However, CS can be different between ASGCM and CGCM. Therefore we use the CGCM in this study. Since the net radiation balance at top of atmosphere (TOA) will alter when physics parameters are swept, resulting in climate drifts in CGCM, flux corrections were applied in previous PPE studies. However, flux corrections may affect CS. In this study, we developed a new method to prevent climate drifts in the PPE experiments of CGCM without flux corrections. We simultaneously swept 10 parameters in atmosphere and surface schemes. The range of CS (estimated from our 35 ensemble members so far) was not wide (2.2K-3.4K). The shortwave cloud (SWcld) feedback relating to changes in middle-level cloud albedo dominated the variations of total feedback. We found three performance metrics of present climate simulations about middle-level cloud albedo, precipitation, and ENSO amplitude that are systematically relating to the variations of SWcld feedback. The observational constrains indicate that the SWcld feedback of standard model is more plausible than other members within this ensemble.
Physics Parameter Ensemble of MIROC5 AOGCM
TOA imbalance changes between AGCM CTL runs with max and min values of each parameter. Based on these imbalances, we can select the set of 10 parameter values having small emulated TOA imbalances. We generate 5000 Latin hypercube samples, and select 100 sets of small emulated TOA imbalances.
CGCM CTL runs with the parameter sets of small emulated TOA imbalances. We succeed to prevent large TOA imbalances and drifts.
Climate sensitivities are estimated by Gregory-style experiments (CTL and 4XCO2 runs). CSs are low and not wide, since the SW cloud feedbacks are always negative.
Climate SensitivityStd model and
uncertainty due to natural variability
SW cloud FDBK
Each model
Differences between 10 more negative SWcloud FDBK models minus 10 less negative SWcld FDBK models.
More negative SWcloud FDBKs are due to more increases of middle-level cloud albedo in the tropical oceans.
Name Name Descriptions
wcbmax CumulusMaximum of cumulus updraft velocity at cloud base [m/s]
precz0 CumulusBase height for cumulus precipitation [m]
clmd Cumulus Entrainment efficiency [ND]
vicec CloudFactor for ice falling speed [m0.474/s]
b1 Cloud Berry parameter [m3/kg]
faz1 TurbulenceFactor for PBL overshooting [ND]
alp1 Turbulence Factor for length scale LT [ND]
tnuw Aerosol Timescale for nucleation [s]
ucmin AerosolMinimum cloud droplet number (liquid) [m−3]
alb Surface Albedo for ice and snow
We simultaneously vary 10 parameters in atmosphere and surface schemes.3 cumulus, 2 cloud, 2 turbulence, 2 aerosol and 1 surface parameters.
Differences of CTL climates between 10 more negative SWcloud FDBK models minus 10 less negative SWcld FDBK models.
SW cloud FDBKs are related to (1)middle-level cloud albedeo(2)precipitation(3)ENSO amplitude
Sou
th m
inus
nor
thS
outh
min
us n
orth
Nin
o3.4
SS
T
Obs.
Obs.
Obs.
Std model
Max ENSO
Min ENSO
Negative corr bet SW cloud FBDKs and these metrics.
The obs constrains indicate that the SW cloud FDBKs of std model is more plausible than others within this ensemble
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