大气热力强迫和动力强迫的调配及平均经圈环流的仿真模拟

通过研究平均经围环流（ＭＭＣ）及其所受的内外强迫作用的相互配置，指出对ＭＭＣ的热力和动力强迫满足确定的调配率。这一调配率受大气内在的斜压性、静力稳定度及绝对涡度制约。利用辐射加热和凝结加热参数化方案，结合欧洲中期天气预报中心（ＥＣＭＷＦ）的分析资料，对１月份平均经围环流进行数值仿真模拟。结果表明，热带对流加热可以形成双层Ｈａｄｌｅｙ环流结构；涡动动量输送对双Ｈａｄｌｅｙ环流的形成也有一定影响。中高纬度的ＭＭＣ则主要由外动量强迫及大气的动量和热量输送特征决定。     

1961～1997年110～140°E垂直经圈环流的年际变化特征及其与海温变化的关系

用 ＮＣＥＰ／ＮＣＡＲ再分析资料，分析了 １９６１～ １９９７各年 １月和 ７月的大气垂直 经圈环流的变化特征，特别分析了１１０～１４０°Ｅ平均的垂直经圈环流和其中的东亚季风环 流。计算了各年的经圈环流与多年平均垂直经圈环流之相似系数、差异系数和相对强度。文 中除讨论了它们的年际和１０年际变化外，还讨论了东亚季风环流强弱变化与ＥＮＳＯ循环的 关系。结果表明：（１）垂直经圈环流除有年变化外，存在着较明显的年际和年代际变化。１ 月的全球平均经圈环流１９６６～１９７４年较弱，１９７６～１９８７年较强；７月的全球垂直经圈环流 则是１９６３～１９７４年较强，１９８６～１９９５年则相对较弱。（２）１１０～１４０°Ｅ的平均经圈环流主要 特点是： １月东亚季风环流圈代替了北半球的Ｆｅｒｒｅｌ环流圈，７月东亚季风环流圈代替了北 半球的Ｈａｄｌｅｙ环流圈，而且其１０年际变化也比较明显。（３）东亚季风环流强弱的变化与 ＥＮＳＯ循环有一定的关系。     

北半球冬季环流异常对我国东北夏季长期天气过程的影响

用北半球１４个冬季的５００ｈＰａ候距平高度场和１４个夏季东北地区温度和降水候距平资料，分析了冬季环流异常对次年夏季温度和降水异常的影响，发现北半球冬季环流异常的显著区与冬季大气活动中心或超长波槽脊相联系；与我国东北地区夏季温度和降水异常关系密切。在Ｅｌ Ｎｉｎｏ和反Ｅｌ Ｎｉｎｏ年，这种现象更为明显。     

“六月突变”前后大气环流对太平洋海温异常响应的数值试验

采用中国科学院大气物理研究所大气环流模式的持续积分方案，模拟了４，５，６三个月大气环流对正常，异常海温强迫的响应。结果表明，持续积分结果较通常积分结果约提前一个月，蓁特点保持不变，因此，提出了利用ＧＣＭ制作月预报的可能途径。     

西太平洋暖池次表层海温一场与ENSO关系的CGCM模拟结果

全球大气与热带太平洋相耦合的数值模式（ＣＧＣＭ） 很好地模拟了ＥＮＳＯ （ 厄尔尼诺和拉尼娜） 型海表水温（ＳＳＴ） 异常, 进一步分析多年的模式积分结果, 清楚地表明赤道中东太平洋ＳＳＴ 异常与西太平洋暖池次表层（ 深１００ ～２００ ｍ） 的海温异常有密切的关系。在Ｅｌ Ｎｉｎｏ 事件发生之前的半年到一年左右, 西太平洋暖池次表层海温有明显正异常,并向东传播; 而在Ｌａ Ｎｉｎａ 发生之前的半年到一年左右, 暖池次表层海温有明显负异常, 并向东传播。因此, 西太平洋暖池次表层海温异常及其东传对Ｅｌ Ｎｉｎｏ （Ｌａ Ｎｉｎａ） 的发生有极重要作用。     

1991年江淮暴雨期间环流异常的动力延伸预报试验

介绍了利用Ｔ４２Ｌ９模式对１９９１年夏季江淮流域暴雨期间旬和月平均环流异常的动力延伸预报（ＤＥＲＦ）试验和利用ＯＳＵ－ＡＧＣＭ进行青藏高原热力异常敏感性试验的结果，指出Ｔ４２Ｌ９模式对造成暴雨的环流异常有一定的预报能力，并证实高原的热力异常是引起江淮暴雨的一个重要因子。     

一个耦合了简化生物圈方案的全球大气环流谱模式及其性能测试

在美国ＮＭＣ ＡＧＣＭ模式的基础上，参照ＣＯＬＡ低分辨率ＡＧＣＭ模式，移植和改进了一个包括植被层陆面过程的陆－气耦合全球大气环流谱模式。其水平分辨率为菱形截断１５波，垂直方向分为９层，陆面过程采用简化的简单生物圈模式。     

极冰气候效应的数值试验

利用一个大气环流模式（ＡＧＣＭ）和一个全球耦合海气模式（ＣＯＡＧＣＭ）,模拟了北极海冰边界范围的变化对月平均气候的影响。结果表明,极冰边缘的异常完全可以改变中高纬度某些地区的局地气候。受冷源的影响,北半球中高纬度冷高压加强,低纬度暖高压减弱。同时利用一个全球三维大气环流模式,作了海冰反照率参数化的数值试验,用两种不同的海冰反照率参数化方案,检验对地表面温度、海平面气压、极地表面对太阳辐射吸收的影响。模拟试验表明了冰雪圈反照率的反馈作用,对气候变化的影响十分重要。     

热带大气季节内振荡激发El Nino的机制

资料分析了表明,热带大气季节内振荡同Ｅｌ Ｎｉｎｏ发生有密切的关系。在Ｅｌ Ｎｉｎｏ事件发生之前,热带大气（尤其是赤道西太平洋地区）季节内振荡异常加强;伴随着Ｅｌ Ｎｉｎｏ的发生,热带大气季节内振荡动能明显增加。简单海－气耦合模式的分析表明,只有在年陵时间尺度大气外强迫作用下,海－气系统才可以产生类似ＥＮＳＯ模的耦合波。资料和理论模式分析和结果相结合,说明热带大气季节内振荡激发Ｅｌ Ｎｉｎｏ的机制     

大气环流的奇偶对称性（Ⅱ）度量方法和异常分析

本文首先给出南，北半球环流奇，偶对笱分量的绝对，相对度量方法，用它分析了１９８０－１９８６年月平均５００ｈＰａ高度场中奇，偶对称分量的季节变化和年际异常。结果表明：重大ＥｌＮｉｎｏ事件事件与全球月平均环流奇，偶对称分量的异常存在明显联系，环流偶对称分量的异常与ＥｌＮｉｎｏ事件盛期准同时出现、奇对称分量的异常在ＥＩ Ｎｉｎｏ事件发生半年出现。     

热带大气垂直环流对海表温度异常的响应——一个初步的理论分析

本文提出了一个β平面定常的线性二维模式,并考虑了海面边界层和赤道侧向边界层,讨论了热带海表温度异常对大气所产生的垂直环流——经向环流和纬向环流。结果表明:热带大洋东部(例如太平洋)海表温度比平均状态暖而西部较冷时,其上空经向环流(Hadley环流)比平均状态强,而纬向环流(如在太平洋上,称Walker环流)弱。相反,当热带大洋西部暖而东部冷时,经向环流减弱,纬向环流加强。这些是与观测事实比较一致的。     

ENSO, IOD and Indian Summer Monsoon in NCEP climate forecast system

El Ni?o-Southern Oscillation (ENSO), Indian Ocean Dipole (IOD) and Indian Summer Monsoon rainfall features are explored statistically and dynamically using National Centers for Environment Prediction (NCEP) Climate Forecast System (CFSv1) freerun in relation to observations. The 100?years of freerun provides a sufficiently long homogeneous data set to find out the mean state, periodicity, coherence among these climatic events and also the influence of ENSO and IOD on the Indian monsoon. Differences in the occurrence of seasonal precipitation between the observations and CFS freerun are examined as a coupled ocean–atmosphere system. CFS simulated ENSO and IOD patterns and their associated tropical Walker and regional Hadley circulation in pure ENSO (PEN), pure IOD (PIO) and coexisting ENSO-IOD (PEI) events have some similarity to the observations. PEN composites are much closer to the observation as compared to PIO and PEI composites, which suggest a better ENSO prediction and its associated teleconnections as compared to IOD and combined phenomenon. Similar to the observation, the model simulation also show that the decrease in the Indian summer monsoon rainfall during ENSO phases is associated with a descending motion of anomalous Walker circulation and the increase in the Indian summer monsoon rainfall during IOD phase is associated with the ascending branch of anomalous regional Hadley circulation. During co-existing ENSO and IOD years, however, the fate of Indian summer monsoon is dictated by the combined influence of both of them. The shift in the anomalous descending and ascending branches of the Walker and Hadley circulation may be somewhat attributed to the cold (warm) bias over eastern (western) equatorial Indian Ocean basin, respectively in the model. This study will be useful for identifying some of the limitations of the CFS model and consequently it will be helpful in improving the model to unravel the realistic coupled ocean–atmosphere interactions for the better prediction of Indian Summer Monsoon.     

Upscale effects in simulations of tropical convection on an equatorial beta-plane

A cloud-resolving model is configured to span the full meridional extent of the tropical atmosphere and have sufficient zonal extent to permit the representation of tropical cloud super-clusters. This is made computationally feasible by the use of anisotropic horizontal grids where one horizontal coordinate direction has over an order of magnitude finer resolution than the other direction. Typically, the meridional direction is chosen to have the coarser resolution (40 km grid spacing) and the zonal direction has enough resolution to ‘permit’ crude convective squall line ascent (1 km grid spacing). The aim was to run in cloud-resolving model (CRM) mode yet still have sufficient meridional resolution and extent to capture the equatorial trapped waves and the Hadley circulation. The large-scale circulation is driven by imposed uniform tropospheric cooling in conjunction with a fixed sea surface temperature distribution. At quasi-equilibrium the flow is characterized by sub-tropical jetstreams, tropical squall line systems that form eastward-propagating super-clusters, tropical depressions and even hurricanes.Two scientific issues are briefly addressed by the simulations: what forces the Hadley circulation and the nature of stratospheric waves appearing in the simulation. It is found that the presence of a meridional sea surface temperature gradient is not sufficient on its own to force a realistic Hadley circulation even though convection communicates the underlying temperature gradient to the atmosphere. It is shown in a simulation that accounts for the observed time and zonal-mean momentum forcing effect of large-scale eddies (originating in middle latitudes) that the heaviest precipitation is concentrated near the equator in association with moisture flux convergence driven by the Trade winds.A spectral analysis of the stratospheric waves found on the equator using the dispersion relation for equatorially-trapped waves provides strong evidence for the existence of a domain-scale Kelvin wave together with eastward and westward propagating inertia-gravity waves. The eastward-propagating stratospheric waves appear to be part of a convectively coupled wave system travelling at about 15 ms⁻¹.     

Upscale effects in simulations of tropical convection on an equatorial beta-plane

A cloud-resolving model is configured to span the full meridional extent of the tropical atmosphere and have sufficient zonal extent to permit the representation of tropical cloud super-clusters. This is made computationally feasible by the use of anisotropic horizontal grids where one horizontal coordinate direction has over an order of magnitude finer resolution than the other direction. Typically, the meridional direction is chosen to have the coarser resolution (40 km grid spacing) and the zonal direction has enough resolution to ‘permit’ crude convective squall line ascent (1 km grid spacing). The aim was to run in cloud-resolving model (CRM) mode yet still have sufficient meridional resolution and extent to capture the equatorial trapped waves and the Hadley circulation. The large-scale circulation is driven by imposed uniform tropospheric cooling in conjunction with a fixed sea surface temperature distribution. At quasi-equilibrium the flow is characterized by sub-tropical jetstreams, tropical squall line systems that form eastward-propagating super-clusters, tropical depressions and even hurricanes.Two scientific issues are briefly addressed by the simulations: what forces the Hadley circulation and the nature of stratospheric waves appearing in the simulation. It is found that the presence of a meridional sea surface temperature gradient is not sufficient on its own to force a realistic Hadley circulation even though convection communicates the underlying temperature gradient to the atmosphere. It is shown in a simulation that accounts for the observed time and zonal-mean momentum forcing effect of large-scale eddies (originating in middle latitudes) that the heaviest precipitation is concentrated near the equator in association with moisture flux convergence driven by the Trade winds.A spectral analysis of the stratospheric waves found on the equator using the dispersion relation for equatorially-trapped waves provides strong evidence for the existence of a domain-scale Kelvin wave together with eastward and westward propagating inertia-gravity waves. The eastward-propagating stratospheric waves appear to be part of a convectively coupled wave system travelling at about 15 ms⁻¹.     

热带太平洋、印度洋海温异常对处于厄尔尼诺事件成熟期的东亚Hadley环流的影响

分析了热带太平洋El Nino事件和热带印度洋海盆一致的暖海温异常事件（记为暖海盆模态）与东亚Hadley环流的关系及海温异常对东亚Hadley环流的影响。结果表明：（1）东亚Hadley环流与El Nino循环的关系密切,El Nino事件从开始到消亡的不同位相期,东亚地区表现为随位相变化的异常经向垂直环流,在El Nino成熟期由异常顺时针经向环流圈转换为异常逆时针经向环流圈,意味着东亚Hadley环流圈的显著减弱。（2）冬季Nino3指数、赤道印度洋海盆一致型模态指数（IOBMI）与东亚Hadley环流指数间呈负相关关系,相关系数分别为-0.42、-0.39,远超过0.01信度的显著性检验,表明当El Nino事件和印度洋暖海盆模事件发生时,东亚Hadley环流减弱。模拟结果与诊断分析结果一致。（3）鉴于印度洋海盆模态和太平洋El Nino事件的密切联系,在考虑冬季东亚Hadley环流变化时,应考虑El Nino事件和印度洋海盆一致型海温异常事件的共同作用。数值试验结果表明两大洋的共同作用会产生更强的东亚异常逆时针经向垂直环流,使得东亚Hadley环流显著减弱。     

ANOMALIES OF THE BACKGROUND CIRCULATION OF THE IAP GCM MODEL ATMOSPHERE IN AN EL NINO YEAR

Analysis is performed of the May-September mean circulation,referred to as the background circulationhereinafter,in the IAP(Institute of Atmospheric Physics,Academia Sinica)GCM model atmosphere,It is foundthat in an El Nino year there occur anomalies in a set of major systems,e.g.,Southetm Oscillation,Walker andHadley circulations,the western Pacific subtropical high and ITCZ,2nd in large-scale precipitation,with theirhappening dominantly in the Northern Hemisphere tropical and subtropical latitudes in the western Pacific.These results that are in rough agreement with the analyz(?)d actual observations demonstrate the applicabilities ofthe model to the study of low-latitude circulations.     

Climate sensitivity to changes in solar insolation in a simple coupled climate model

A simple coupled ocean, atmosphere and sea-ice model is presented. The idealised model consists of a zonally averaged land and ocean strip of constant angular width extending from pole to pole. The meridional energy transport in the ocean is modelled by contributions from the large scale thermohaline overturning cells and from horizontal diffusive fluxes. The atmospheric meridional energy transports are parametrised as diffusive fluxes in addition to advective transports in the Hadley domain. This parametrisation resolves the equatorward moisture transport as well as the poleward transport of potential energy in the upper branch of the Hadley circulation. The model reproduces the annual averaged meridional energy transports in the climate system with a small number of free model parameters. The basic feedbacks between the three climatic components are studied by investigating the model's sensitivity towards reductions in the solar insolation. It is found that the meridional energy transport in the ocean does not amplify the ice albedo feedback. This has important implications for modelling the climate sensitivity in atmosphere-only models, as these would exaggerate the sensitivity to changes in the solar insolation if their parametrisations of the meridional energy transport are constrained by surface temperatures. The role of the dependence of the atmospheric transports on the meridional temperature gradient is shown to have a significant influence on the sensitivity on the coupled model, and the inclusion of seasonal cycles greatly increase the models sensitivity. The Hadley circulation does significantly alter the strength of the ice-albedo feedback in the coupled model. The idealised configuration of the model makes it a useful tool for studying the feedbacks in the ocean-atmosphere-sea ice system in the context of the "Snowball Earth" hypothesis.     

IAP GCM模式大气背景环流在厄尔尼诺年的异常

本文分析了中国科学院大气物理研究所大气环流模式(IAP GCM)模式大气5～9月平均环流(本文称为背景环流)。结果表明;厄尔尼诺年一系列重要系统(南方涛动、瓦克环流、哈德莱环流、西太平洋副热带高压和热带辐合带)及大范围降水均发生明显异常;北半球西太平洋热带、副热带是环流异常的主要区域。它们与观测资料的分析结果基本一致,从而论证了该模式在低纬环流研究中的应用前景。     

1948-2004年全球平均Hadley环流强度指数与特征

利用NCEP/NCAR逐月平均风场资料,研究了全球平均Hadley环流特征.利用3层4个关键区的风定义并计算了1948年1月-2004年12月的全球纬向平均的南/北半球和全球Hadley环流逐月强度指数.结果表明:计算的Hadley环流指数可以合理地表示Hadley环流的强度;北半球Hadley环流除7-9月(南半球除5月)外都呈增强趋势;南/北半球的年平均Hadley环流也是增强的.年际相关分析表明:Hadley环流指数与SOI有非常高的负相关,Hadley环流强度的年际变化与ENSO关系密切.