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1.
热带大气季节内振荡数值模拟对积云对流参数化方案的敏感性 总被引：4，自引：0，他引：4
利用中国科学院大气物理研究所大气科学和地球流体力学数值模拟国家重点实验室(LASG)的大气环流模式(SAMIL-R42L9)研究了热带大气季节内振荡(MJO)的模拟对积云对流参数化方案的敏感性,结果表明两种对流参数化方案——湿对流调整方案(MCA)和Zhang-McFarlane(1995年)方案对MJO的模拟能力有明显的差异。MCA方案较好地模拟出了MJO的基本特征,包括季节内的时间尺度和向东的传播。Zhang-McFarlane(1995年)对流方案模拟的MJO振幅非常弱,而且缺乏连续的传播特征,在MJO的演变过程中弱的低层水汽辐合使MJO难以维持和传播。两种不同的对流参数化方案产生的非绝热加热垂直廓线明显不同,Zhang-McFarlane(1995年)方案产生的非绝热加热强度在对流层各层过于一致,没有明显的最大加热层,而且平均的加热强度太弱,这是该方案难以模拟出合理的MJO的主要原因之一。因此,模式对热带大气季节内振荡的模拟能力很大程度上依赖于所使用的积云对流参数化方案,当积云参数化方案改变时模式模拟的MJO也发生明显变化,而非绝热加热廓线是对流参数化方案影响MJO模拟的一个重要影响因子。3种不同的非绝热加热垂直分布的敏感性试验表明,当最大的加热层位于对流层中低层尤其是对流层中层时,更容易产生出与观测较为接近的季节内的扰动,而当最大加热位于对流层高层时,更易于激发出西传的扰动。 相似文献
2.
北京气候中心大气模式对季节内振荡的模拟 总被引：7，自引：1，他引：6
对北京气候中心大气模式(BCC AGCM2.0.1)模拟热带季节内振荡的能力进行了检验.北京气候中心新一代气候模式(BCC AGCM2.0.1)是在原中国国家气候中心模式的基础上参考NCAR CAM3改进形成的.新模式中引进了一个新的参考大气和参考面气压.因此原模式的预报量中的气温(T)和地面气压(p_s)则变为它们对参考大气气温的偏差和对参考面气压的偏差.模式还加入了新的Zhang-Mcfarlane对流参数化方案,并对其参数计算方法进行调整和改进.此外还对模式边界层处理、雪盖计算等进行了改进.上述模式在实测的月海温作为下边界条件的情况下运行52年(1949年9月-2001年10月).然后对运行结果中的季节内振荡的状况进行分析,主要结果如下:NCAR CAM3模式模拟热带季节内振荡的能力很差,主要表现在模拟的热带季节内振荡强度很弱;东移波与西移波的强度很接近,而实际观测中是东移波的能量要远大于西移波;季节内振荡的季节变化及空间分布与观测相差很远.北京气候中心大气模式(BCC AGCM2.0.1)模拟热带季节内振荡的能力有显著的提高.模拟的热带季节内振荡很明显,强度接近于观测结果;模拟东移波的能量要大于西移波,这与观测较为一致;季节内振荡的季节变化和空间分布与观测相差不大.总的来看,BCC AGCM2.0.1模式在模拟热带季节内振荡方面比CAM3模式有明显的改进. 相似文献
3.
大气季节内振荡的数值模拟比较研究 总被引：13，自引：0，他引：13
用国内外两个较好的大气环流模式、在观测海表温度的强迫下进行了长时间(1978—1989年)的数值积分,然后对数值模拟结果与NCAR/NCEP再分析资料进行比较分析,其结果清楚表明,模式模拟结果的均方根误差中有30%—40%是来自于模拟的大气季节内振荡的均方根误差。尤其是,大气季节内振荡模拟的均方根误差的分布形势与总的均方根误差的分布形势几乎完全一致。对热带地区大气季节内振荡动能的模拟结果与NCAR/NCEP再分析资料的比较分析表明,其差异也十分明显,说明模式对热带大气季节内振荡的模拟能力也还比较差。因此可以认为,大气季节内振荡在天气气候模拟中极为重要,而如何在数值模式中模拟好大气季节内振荡还需要进行很好地研究。 相似文献
4.
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。 相似文献
5.
大气环流模式IAP AGCM4.0对东亚高空副热带西风急流的模拟及偏差原因分析 总被引：1，自引：1，他引：0
基于中国科学院大气物理所大气环流模式IAP AGCM4.0总共30年(1979~2008年)的AMIP(大气环流模式比较计划)数值模拟试验结果,评估了模式对东亚高空副热带西风急流的模拟能力,分析了模式模拟偏差的可能原因,以及不同对流参数化方案对模拟结果的影响。结果表明,IAP AGCM4.0可以较好地模拟出东亚高空副热带西风急流冬季和夏季的空间结构及其季节变化特征;与JRA-25再分析资料相比,模式模拟的急流强度总体偏弱;就急流位置而言,模式模拟的急流位置冬季略偏南,夏季则相对偏北;模式可以较好地模拟出夏季西风急流的季节内演变特征,包括夏季西风急流位置逐月北跳的特征,只是模式模拟的逐月西风急流位置仍偏北。夏季200 h Pa纬向风EOF分解结果表明,模式模拟和再分析资料的EOF第一模态空间型态较为接近,均反映了西风急流的年际变化特征,但两者的时间系数相关较小,表明模式对西风急流南北位置年际变化的模拟偏差较大。针对模式模拟的地表感热通量及对流层中上层经向温度差(MTD)的分析结果表明,模式对阿拉伯半岛东南部、阿拉伯海西北部及印度北部的地表感热通量的模拟存在偏差,影响到对流层中高层温度场、高度场的模拟,使得IAP AGCM4.0模拟的MTD强度较再分析资料相对偏弱,MTD变化最大的区域位置相对偏北,且模式模拟的MTD年际变化与再分析资料相比也有较大偏差,从而造成模式对西风急流模拟的偏差。此外,不同积云对流参数化方案也可影响对流层中上层经向温度差的模拟,进而影响模式对东亚高空副热带西风急流的模拟。 相似文献
6.
中国热带大气季节内振荡研究进展 总被引：7，自引：1，他引：6
热带大气季节内振荡(包括MJO)是大气环流的重要系统,它的活动及异常既对其他系统有一定的作用,也对长期天气和短期气候有明显影响。因此,热带大气季节内振荡一直是大气科学的前沿研究课题之一。文中对近5—10年中国学者的有关研究工作及其进展做了简要回顾和综合,主要包括:(1)热带大气季节内振荡特别是MJO的动力学机制;(2)热带大气季节内振荡以及MJO的数值模拟问题,特别是大气非绝热加热廓线对模式模拟MJO的重要作用;(3)热带大气季节内振荡和MJO,特别是在赤道西太平洋地区,与ENSO的相互作用关系;(4)热带大气季节内振荡(包括MJO)及其流场形势对西太平洋台风活动的重要影响,即MJO对西北太平洋台风生成数的调制作用,以及热带大气季节内低频气旋性(LFC)和反气旋性(LFAC)流场对西太平洋台风路径的影响;(5)热带大气季节内振荡(包括MJO)的活动及异常对东亚和南亚夏季风建立、活动异常的影响,以及它们与中国降水异常的密切关系。 相似文献
7.
基于1979—2000年的NCEP/NCAR海平面气压和位势高度场资料分析了南半球大气环流的准半年振荡 (半年波) 现象。结果表明:这一现象主要出现在南半球对流层低层的中高纬度和中高层的热带地区。对南半球热带外大气而言, 40°S和65°S是低层大气环流准半年振荡最为显著的两个纬度带, 半年波的贡献都超过了70%, 低层南半球中高纬度海平面气压场季节变化的反位相也主要体现为各自半年波分量变化的反位相。在此基础上, 检验了IAP 9L AGCM (大气物理研究所9层大气环流模式) 对这一现象模拟的能力, 模拟结果显示, 模式成功模拟了65°S处海平面气压场的准半年振荡现象, 其振幅略低于观测结果, 但模式对40°S处气压场准半年振荡的模拟效果较差。 相似文献
8.
热带大气季节内振荡的传播及影响因子研究 总被引：15，自引：2，他引：13
通过观测资料的分析,对热带大气季节内振荡(ISO)的传播(移动)进行了深入系统的研究,揭示了热带大气ISO的纬向和经向移动的特征,以及热带大气低频动能的跨赤道传播特征.同时,通过对比分析还揭示了ENSO和热带对流加热场异常对热带大气ISO移动的影响. 相似文献
9.
蒸发－风反馈机制的进一步研究 总被引：6，自引：2，他引：4
对蒸发-风反馈的作用进行了简单动力学研究。结果表明,蒸发-风反馈不能像波动-CISK那样改变热带大气波动的性质(减缓移速),不可能单独成为激发热带大气季节内振荡的动力学机制。在积云对流加热和蒸发-风反馈的共同作用下,CISK-Kelvin波和CISK-Rossby波可以不稳定发展,共同作用比单独的积云对流加热反馈作用能更全面合理地解释热带大气季节内振荡的活动。因此,蒸发-风反馈对于热带大气季节内振荡也有重要作用。 相似文献
10.
MJO对中国春季降水影响的数值模拟研究 总被引：2，自引：0，他引：2
利用IAP-AGCM4.0模式,通过多初值集合数值模拟研究了赤道附近的大气季节内振荡(MJO)传播的两个关键位相期对中国东部春季降水的影响.当在赤道中东印度洋及赤道西太平洋引进异常非绝热加热(强MJO活动)强迫时,模式很好地模拟出了中国东部地区春季降水的异常形势,模式模拟与先期所作的诊断分析结果极为相似,即在MJO的第2-3(6-7)位相,中国长江中下游地区多雨(中国东部大部分地区降水偏少).对模式输出的高度场、风场、散度和涡度场以及水汽输送场的分析表明,中国春季降水异常的发生分别与异常非绝热加热在东亚/西北太平洋地区所造成的异常大气环流形势密切相关.对逐日响应场的分析表明,就MJO活动影响中国春季降水的可能物理过程及机制进行的讨论表明,赤道附近的异常对流加热不仅可以在赤道附近激发产生大气的罗斯贝波和开尔文波型响应,而且,还会在大气中激发产生从热带到中高纬度的罗斯贝波列遥响应.但是,由于异常对流加热发生的地区不同,大气遥响应场的形势也会十分不同,它所导致的影响也就很不一样.当异常对流加热发生在赤道中东印度洋(对应MJO的第2-3位相)时,大气的罗斯贝波列遥响应将在东亚/西太平洋地区形成有利于中国东部(尤其是长江中下游地区)春季降水偏多的形势;当异常对流加热发生在赤道西太平洋(对应MJO的第6-7位相)时,大气的罗斯贝波列遥响应将在东亚/西太平洋地区形成不利于中国东部春季降水的形势. 相似文献
11.
Sensitivity of the Simulated Tropical Intraseasonal Oscillation to Cumulus Parameterizations 
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下载免费PDF全文 The sensitivity of the simulated tropical intraseasonal oscillation or MJO （Madden and Julian oscillation） to different cumulus parameterizations is studied by using an atmospheric general circulation model （GCM）--SAMIL （Spectral Atmospheric Model of IAP LASG）. Results show that performance of the model in simulating the MJO alters widely when using two different cumulus parameterization schemes-the moist convective adjustment scheme （MCA） and the Zhang-McFarlane （ZM） scheme. MJO simulated by the MCA scheme was found to be more realistic than that simulated by the ZM scheme. MJO produced by the ZM scheme is too weak and shows little propagation characteristics. Weak moisture convergence at low levels simulated by the ZM scheme is not enough to maintain the structure and the eastward propagation of the oscillation. These two cumulus schemes produced different vertical structures of the heating profile. The heating profile produced by the ZM scheme is nearly uniform with height and the heating is too weak compared to that produced by the MCA, which maybe contributes greatly to the failure of simulating a reasonable MJO. Comparing the simulated MJO by these two schemes indicate that the MJO simulated by the GCM is highly sensitive to cumulus parameterizations implanted in. The diabatic heating profile plays an important role in the performance of the GCM. Three sensitivity experiments with different heating profiles are designed in which modified heating profiles peak respectively in the upper troposphere （UH）, middle troposphere （MH）, and lower troposphere （LH）. Both the LH run and the MH run produce eastward propagating signals on the intraseasonal timescale, while it is interesting that the intraseasonal timescale signals produced by the UH run propagate westward. It indicates that a realistic intraseasonal oscillation is more prone to be excited when the maximum heating concentrates in the middle-low levels, especially in the middle levels, while westward propagating disturbances 相似文献
12.
Sensitivity of the Simulated Tropical Intraseasonal Oscillation to Cumulus Parameterizations 下载免费PDF全文
下载免费PDF全文 The sensitivity of the simulated tropical intraseasonal oscillation or MJO (Madden and Julian oscilla tion)to different cumulus parameterizations is studied by using an atmospheric general circulation model (GCM)-SAMIL(Spectral Atmospheric Model of IAP LASG).Results show that performance of the model in simulating the MJO alters widely when using two different cumulus parameterization schemes-the moist convective adjustment scheme(MCA)and the Zhang-McFarlane(ZM)scheme.MJO simulated by the MCA scheme was found to be more realistic than that simulated by the ZM scheme.MJO produced by the ZM scheme is too weak and shows little propagation characteristics.Weak moisture convergence at low levels simulated by the ZM scheme is not enough to maintain the structure and the eastward propagation of the oscillation.These two cumulus schemes produced different vertical structures of the heating profile.The heating profile produced by the ZM scheme is nearly uniform with height and the heating is too weak compared to that produced by the MCA,which maybe contributes greatly to the failure of simulating a reasonable MJO.Comparing the simulated MJO by these two schemes indicate that the MJO simulated by the GCM is highly sensitive to cumulus parameterizations implanted in.The diabatic heating profile plays an important role in the performance of the GCM.Three sensitivity experiments with different heating profiles are designed in which modified heating profiles peak respectively in the upper troposphere(UH), middle troposphere(MH),and lower troposphere(LH).Both the LH run and the MH run produce eastward propagating signals on the intraseasonal timescale,while it is interesting that the intraseasonal timescale signals produced by the UH run propagate westward.It indicates that a realistic intraseasonal oscillation is more prone to be excited when the maximum heating concentrates in the middle-low levels,especially in the middle levels,while westward propagating disturbances axe more prone to be produced when the maximum heating appears very high. 相似文献
13.
Xiaolong Jia Chongyin Li Ningfang Zhou Jian Ling 《Dynamics of Atmospheres and Oceans》2010,49(2-3):141-163
The Madden–Julian oscillation (MJO) is simulated using an AGCM with three different cumulus parameterization schemes: a moist convective adjustment (MCA) scheme, the Zhang–McFarlane (ZM) mass-flux scheme, and the Tiedtke scheme. Results show that the simulated MJO is highly dependent on the cumulus parameterization used. Among the three cumulus parameterizations, only the MCA scheme produces MJO features similar to observations, including the reasonable spatial distribution, intraseasonal time scales and eastward propagation. Meanwhile, the amplitude is too large and the eastward propagation speed too fast than observations and the relationship between precipitation and low-level wind anomaly is unrealistic with enhanced convection occurring within easterly anomalies instead of westerly anomalies as in observations. The over-dependence of precipitation on boundary convergence produced by the MCA scheme is presumably responsible for this unrealistic phase relation in the simulation. The other two schemes produce very poor simulations of the MJO: spectral power of westward propagation is larger than that of eastward propagation in zonal wind and precipitation, indicating a westward propagation of the intraseasonal variability.The mean state and vertical profile of diabatic heating are perhaps responsible for the differences in these simulations. The MCA scheme produces relatively realistic climate background. When either ZM or Tiedtke scheme is used, the observed extension of westerly winds from the western Pacific to the dateline is missing and precipitation over the equatorial region and SPCZ is dramatically underestimated. In addition, diabatic heating produced by both ZM and Tiedtke schemes are very weak and nearly uniform with height. The heating profile produced by the MCA scheme has a middle-heavy structure with much larger magnitude than those produced by the other two schemes. In addition, a very unrealistic boundary layer heating maximum produced by the MCA scheme induces too strong surface convergence, which perhaps contributes to the too strong intraseasonal variability in the simulation. 相似文献
14.
Sensitivity of MJO simulations to diabatic heating profiles 总被引：2，自引：0，他引：2
The difficulty for global atmospheric models to reproduce the Madden–Julian oscillation (MJO) is a long-lasting problem. In an attempt to understand this difficulty, simple numerical experiments are conducted using a global climate model. This model, in its full paramterization package (control run), is capable of producing the gross features of the MJO, namely, its planetary-scale, intraseasonal, eastward slow propagation. When latent heating profiles in the model are artificially modified, the characteristics of the simulated MJO changed drastically. Intraseasonal perturbations are dominated by stationary component over the Indian and western Pacific Oceans when heating profiles are top heavy (maximum in the upper troposphere). In contrast, when diabatic heating is bottom heavy (maximum in the lower troposphere), planetary-scale, intraseasonal, eastward propagating perturbations are reproduced with a phase speed similar to that of the MJO. The difference appears to come from surface and low-level moisture convergence, which is much stronger and more coherent in space when the heating profile is bottom heavy than when it is top heavy. These sensitivity experiments, along with other theoretical, numerical, and observational results, have led to a hypothesis that the difficulty for global models to produce the MJO partially is rooted in a lack of sufficient diabatic heating in the lower troposphere, presumably from shallow convection. 相似文献
15.
The performance of ECHAM5 atmospheric general circulation model (AGCM) is evaluated to simulate the seasonal mean and intraseasonal variability of Indian summer monsoon (ISM). The model is simulated at two different vertical resolutions, with 19 and 31 levels (L19 and L31, respectively), using observed monthly mean sea surface temperature and compared with the observation. The analyses examine the biases present in the internal dynamics of the model in simulating the mean monsoon and the evolution of the boreal summer intraseasonal oscillation (BSISO) and attempts to unveil the reason behind them. The model reasonably simulates the seasonal mean-state of the atmosphere during ISM. However, some notable discrepancies are found in the simulated summer mean moisture and rainfall distribution. Both the vertical resolutions, overestimate the seasonal mean precipitation over the oceanic regions, but underestimate the precipitation over the Indian landmass. The performance of the model improves with the increment of the vertical resolution. The AGCM reasonably simulates some salient features of BSISO, but fails to show the eastward propagation of the convection across the Maritime Continent in L19 simulation. The propagation across the Maritime Continent and tilted rainband structure improve as one moves from L19 to L31. The model unlikely shows prominent westward propagation that originates over the tropical western Pacific region. L31 also produces some of the observed characteristics of the northward propagating BSISOs. However, the northward propagating convection becomes stationary in phase 5–7. The simulation of shallow diabatic heating structure and the heavy rainfall activity over the Bay of Bengal indicate the abundance of the premature convection-generated precipitation events in the model. It is found that the moist physics is responsible for the poor simulation of the northward propagating convection anomalies. 相似文献
16.
In this study, satellite-derived outgoing longwave radiation (OLR) and the reanalysis from the National Centers for Environmental
Prediction/National Center for Atmospheric Research are used as verification data in a study of intraseasonal variability
in the Goddard Laboratory for Atmospheres (GLA) and the United Kingdom Meteorological Office (UKMO) atmospheric general circulation
models. These models simulated the most realistic intraseasonal oscillations (IO) of the 15 Atmospheric Model Intercomparison
Project models previously analyzed. During the active phase of the intraseasonal oscillation, convection is observed to migrate
from the Indian Ocean to the western/central Pacific Ocean, and into the South Pacific Convergence Zone (SPCZ). The simulated
convection, particularly in the GLA model, is most realistic over the western/central Pacific Ocean and the SPCZ. In the reanalysis,
the baroclinic structure of the IO is evident in the eddy-stream function, and eastward migration of the anticyclone/cyclone
pairs occurs in conjunction with the eastward development of convection. Both the GLA and UKMO models exhibit a baroclinic
structure on intraseasonal time scales. The GLA model is more realistic than the UKMO model at simulating the eastward migration
of the anticyclone/cyclone pairs when the convection is active over the western/central Pacific. In the UKMO model, the main
heating is located off the equator, which contributes to the irregular structures seen in this model on intraseasonal time
scales. The maintenance and initiation of the intraseasonal oscillation has also been investigated. Analysis of the latent
heat flux indicates that evaporative wind feedback is not the dominant mechanism for promoting the eastward propagation of
the intraseasonal oscillation since evaporation to the west of the convection dominants. The data suggest a wave-CISK (conditional
instability of the secondkind) type mechanism, although the contribution by frictional convergence is not apparent. In the
GLA model, enhanced evaporation tends to develop in-place over the west Pacific warm pool, while in the UKMO simulation westward
propagation of enhanced evaporation is evident. It is suggested that lack of an interactive ocean may be associated with the
models systematic failure to simulate the eastward transition of convection from the Indian Ocean into the western Pacific
Ocean. This hypothesis is based upon the examination of observed sea surface temperature (SST) and its relationship to the
active phase of the intraseasonal oscillation, which indicates that the IO may evolve as a coupled ocean-atmosphere mode.
The eastward propagation of convection appears to be related to the gradient of SST, with above normal SST to the east of
the convection maintaining the eastward evolution, and decreasing SST near the western portion of the convective envelope
being associated with the cessation of convection.
Received: 13 September 1996/Accepted: 14 April 1997 相似文献
17.
Jian Ling Chongyin Li Wen Zhou Xiaolong Jia 《Theoretical and Applied Climatology》2014,115(1-2):231-241
Mechanisms for convective initiation of the Madden–Julian oscillation (MJO) remain poorly understood. During recent years, <50 % of large-scale convectively active episodes over the tropical Indian Ocean have led to MJO initiation. This study explores the structure and evolution of precipitation, diabatic heating, and potential vorticity (PV) that might be used to tell whether an MJO event will be initiated once such a convection episode occurs. Three different cases are studied. As convection becomes active in a large area over the tropical Indian Ocean, early signs favorable for MJO initiation are apparent: a persistent basin-scale coverage in the zonal direction by positive anomalies in precipitation and diabatic heating (in a swallowtail pattern), a persistent vertical dipole of PV generation with cyclonic (anticyclonic) PV generation in the lower (upper) troposphere covering a zonally extended area, and a cyclonic PV anomaly in the midtroposphere with a cyclonic PV pair straddling the equator immediately west of the diabatic heating center. All these signs are robust in the MJO composite but rarely occur all together in a given MJO case. The likelihood of an MJO event following a convective episode over the tropical Indian Ocean depends on how many of these signs occur and how persistent they are. While a preexisting MJO signal is neither a necessary nor a sufficient sign for MJO initiation, an active convective episode over the tropical Indian Ocean is necessary but insufficient for MJO initiation. MJO initiation depends on detailed convective behaviors over the tropical Indian Ocean. 相似文献
18.
Madden-Julian Oscillations (MJO) in six integrations using an AGCM with different cumulus
parameterization schemes and resolutions are examined to investigate their impacts on the MJO simulation.
Results suggest that the MJO simulation can be affected by both resolution and cumulus parameterization,
though the latter, which determines the fundamental ability of the AGCM in simulating the MJO and the
characteristics of the simulated MJO, is more crucial than the former. Model resolution can substantially
affect the simulated MJO in certain aspects. Increasing resolution cannot improve the simulated MJO
substantially, but can significantly modulate the detailed character of the simulated MJO; meanwhile, the
impacts of resolution are dependent on the cumulus parameterization, determining the basic features of the
MJO. Changes in the resolution do not alter the nature of the simulated MJO but rather regulate the
simulation itself, which is constrained by cumulus parameterization schemes. Therefore, the vertical
resolution needs to be increased simultaneously. The vertical profile of diabatic heating may be a crucial
factor that is responsible for these different modeling results. To a large extent, it is determined by the
cumulus parameterization scheme used. 相似文献