Extending the atmospheric model top to high altitude is important for simulation of upper atmospheric phenomena,such as the stratospheric quasi-biennial oscillation.The high-top version of the Institute of Atmospheric Physics Atmospheric General Circulation Model with 91 vertical layers(IAP-AGCML91)extends to the mesopause at about 0.01 hPa(~80 km).The high-top model with a fully resolved stratosphere is found to simulate a warmer stratosphere than the low-top version,except near the South Pole,thus reducing its overall cold bias in the stratosphere,and significantly in the upper stratosphere.This sensitivity is shown to be consistent with two separate mechanisms:larger shortwave heating and larger poleward stratospheric meridional eddy heat flux in the hightop model than in the low-top model.Results indicate a significant influence of vertical resolution and model top on climate simulations in IAP-AGCM.
Zhaoyang ChaiMinghua ZhangQingcun ZengHe ZhangJiangbo JinJinbo XieTing You
IAP AGCM4.1(Institute of Atmospheric Physics Atmospheric General Circulation Model, version 4.1)是中国科学院大气物理研究所自主研发的大气环流模式,也是中科院地球系统模式CAS-ESM1(Chinese Academy of Sciences Earth System Model, version 1)的大气分量模式。本文利用极端气候分析软件TECA(Toolkit for Extreme Climate Analysis),对IAP AGCM4.1模拟的1979~2012年西北太平洋热带气旋(TC)进行了识别与评估。结果表明IAP AGCM4.1模拟的TC空间分布、路径走向与生成源地与观测基本一致,但模拟的TC个数有所低估,仅为观测的36%。基于K-均值聚类方法的分类评估显示,这种低估主要体现在模式对于西北行转向类和西行类TC没有模拟能力。对于近海西—西北行类、西转向类和东转向类TC,模式模拟的个数可分别达到观测的39%,48%和85%,模拟的季节变化与观测的相关系数在0.89~0.91之间,周期误差在1~2天。就TC路径而言,模式对于近海西—西北行类和东转向类TC模拟效果较好,质心经度误差、质心纬度误差和经纬向标准差的模拟误差分别为1%~5%、4%~16%和5~15%。此外,环流合成分析表明模式很好地再现了东转向类TC发生、发展期间环境流场的演变以及副热带高压的变化情况,模拟的副热带高压强度和面积指数与观测的相关系数可达0.89。模式对西北行转向类和西行类TC模拟能力较差的原因可能与模式对副热带高压的模拟偏差有关。
This study evaluates the performance of the Grid-point Atmospheric Model of IAP LASG,version 3(GAMIL3),in simulating the Madden–Julian Oscillation(MJO),based on the CMIP6(phase 6 of the Coupled Model Intercomparison Project)AMIP(Atmospheric Model Intercomparison Project)simulation.Results show that GAMIL3 reasonably captures the main features of the MJO,such as the eastward-propagating signal in the MJO frequency band,the symmetric and asymmetric structures of the MJO,several convectively coupled equatorial waves,and the MJO life cycle.However,GAMIL3 underestimates the MJO amplitude,especially for outgoing longwave radiation,as do most CMIP5 models,and simulates slow eastward propagation.
