Evaluation of Forecasted Southeast Pacific Stratocumulus in the NCAR, GFDL, and ECMWF Models

被引:78
作者
Hannay, Cecile [1 ]
Williamson, David L. [1 ]
Hack, James J. [1 ]
Kiehl, Jeffrey T. [1 ]
Olson, Jerry G. [1 ]
Klein, Stephen A. [2 ]
Bretherton, Christopher S. [3 ]
Koehler, Martin [4 ]
机构
[1] Natl Ctr Atmospher Res, Boulder, CO 80305 USA
[2] Lawrence Livermore Natl Lab, Livermore, CA USA
[3] Univ Washington, Dept Atmospher Sci, Seattle, WA 98195 USA
[4] European Ctr Medium Range Weather Forecasts, Reading RG2 9AX, Berks, England
基金
美国国家科学基金会;
关键词
LARGE-SCALE MODELS; COMMUNITY ATMOSPHERE MODEL; GENERAL-CIRCULATION MODELS; SINGLE-COLUMN MODEL; SHALLOW CUMULUS CONVECTION; MARINE BOUNDARY-LAYER; LIQUID WATER PATH; DIURNAL CYCLE; TROPICAL PACIFIC; CLIMATE MODEL;
D O I
10.1175/2008JCLI2479.1
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Forecasts of southeast Pacific stratocumulus at 20 degrees S and 85 degrees W during the East Pacific Investigation of Climate (EPIC) cruise of October 2001 are examined with the ECMWF model, the Atmospheric Model (AM) from GFDL, the Community Atmosphere Model (CAM) from NCAR, and the CAM with a revised atmospheric boundary layer formulation from the University of Washington (CAM-UW). The forecasts are initialized from ECMWF analyses and each model is run for 3-5 days to determine the differences with the EPIC field observations. Observations during the EPIC cruise show a well-mixed boundary layer under a sharp inversion. The inversion height and the cloud layer have a strong and regular diurnal cycle. A key problem common to the models is that the planetary boundary layer (PBL) depth is too shallow when compared to EPIC observations. However, it is suggested that improved PBL depths are achieved with more physically realistic PBL schemes: at one end, CAM uses a dry and surface-driven PBL scheme and produces a very shallow PBL, while the ECWMF model uses an eddy-diffusivity/mass-flux approach and produces a deeper and better-mixed PBL. All the models produce a strong diurnal cycle in the liquid water path (LWP), but there are large differences in the amplitude and phase when compared to the EPIC observations. This, in turn, affects the radiative fluxes at the surface and the surface energy budget. This is particularly relevant for coupled simulations as this can lead to a large SST bias.
引用
收藏
页码:2871 / 2889
页数:19
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