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1.
对流凝结加热和垂直风切变对行星波垂直传播的影响   总被引:3,自引:0,他引:3  
本文从理论上分析研究了对流凝结加热和垂直风切变对大气行星波垂直传播的影响。结果表明,对流凝结加热有抑制行星波垂直传播的作用;基本气流的西风(正)垂直切变对行星波的垂直传播有利,而东风(负)切变却对行星波的垂直传播有阻碍作用。 进-步分析还发现,垂直风切变对行星波垂直传播的影响以在中高纬度地区更为显著;对流凝结加热对行星波垂直传播的影响在热带地区更值得重视。并且,垂直风切变和对流凝结加热的影响可能是使得大气中板地波导更显著的重要原因之一。   相似文献   

2.
The three-dimensional propagations of the forced stationary planetary waves in a realistic summer current, in which the vertical and horizontal wind shears are included, are discussed by using the refractive index squared of waves in a spherical coordinate system.The results show that there is no polar wave guide in stationary planetary wave propagations in summer. Thus, stationary planetary waves cannot propagate into the stratosphere. However, there are a wave guide pointing from the subtropics toward middle and high latitudes in the troposphere and another wave guide pointing from the lower troposphere at middle latitudes toward the upper troposphere near 30°oN in the forced stationary planetary wave propagations.A linearized, steady-state, quasi-geostrophic 34-level spherical coordinate model with Rayleigh friction and Newtonian cooling, horizontal kinematic thermal diffusivity is used to simulate the wave guides of three-dimensional propagations of stationary planetary waves in summer.  相似文献   

3.
In this paper,a primitive equation linear wave model is used to examine the effects of three-dimen-sional structure of heating field on the behavior of stationary planetary waves in summer and to comparethe roles of different heating functions for the formation and maintenance of summer monsoon circulationin Asia.It is shown that the aloft heating connected with the latent heating,especially the deep condensationheating associated with the cumulus convection in low latitudes,plays a crucial part in the Asian summer mon-soon and the structures of planetary wave responses are quite sensitive to the vertical distribution of heating.  相似文献   

4.
加热场的三维结构对亚洲夏季风环流的影响   总被引:1,自引:0,他引:1  
林本达  张劲松 《气象学报》1989,47(2):156-164
本文利用原始方程线性波模式考察了加热场的三维结构对夏季定常行星波特性的影响;比较了不同加热方式对亚洲夏季风坏流的形成及维持所起的作用。指出与低纬深厚积云对流相联的凝结加热对亚洲夏季风环流所起的重要作用和大气定常行星波响应对加热场的垂直结构的敏感性。  相似文献   

5.
吕克利 《气象学报》1985,43(2):129-136
文中讨论了非定常流场中加热的影响,研究在非绝热加热作用下,行星尺度波动的建立过程及其定常解。  相似文献   

6.
陈英仪  佟建平 《大气科学》1992,16(6):698-706
本文采用实际的大气资料分析了一个正压平均环流距平模式各项的相对重要性.结果表明,单纯考虑初始场的惯性预报的准确率随所取平均时间的增加而迅速下降,并以长波和超长波段最为显著. 加上气候平均风场及地球球面效应等动力因子后的修正的惯性预报,其结果不如纯惯性预报好.而且,所取的平均时间越长,效果越差.加进散度订正因子后,对长波和超长波的预报起明显改进作用, 对平均环流的预报起重要作用的因子是未知的强迫作用项.根据分析,本文提出了提高平均环流预报准确率的可能途径.  相似文献   

7.
本文采用一个关于大气定常波的16层线性化原始方程三维谱模式,研究了冬季平流层大气对于对流层各种定常大尺度热力强迫的响应。研究结果表明,对流层中的热力强迫作用对于冬季平流层中垂直向上传播的行星定常波的维持有显著的贡献,平流层中强迫扰动的水平结构及其与对流层中扰动的差异与加热场的垂直结构有密切的关系。相对于强度和空间结构相同的强迫源而言,中纬强迫对于平流层的作用比低纬强迫更为显著。  相似文献   

8.
Summary Lower tropospheric (1000–500) hPa kinetic energy (KE), temporal variations of KE and nonlinear KE transfer of rotational and divergent flows and energy conversion between them, partitioning further into stationary and transient components in the Fourier spectral domain and the mechanism for the evolution of significant transient waves for the month July 1979 in the latitudinal belt 10° S–30° N are studied.Divergent zonal and eddy KE show their maxima at the lowest level 1000 hPa. Lower tropospheric monsoon motion provides a non-divergent level close to 850 hPa. The daily flow patterns bear little resemblence to the climatology over tropics at 500 hPa. Although the transient mode of synoptic scale waves is stronger than that of planetary scale waves they are comparable. Analysis of energetics over global tropics can get signature of transient activities embedded in the large scale system. Summer momentum flux in the lower troposphere is essentially associated with stationary planetary and transient synoptic scale waves. Waves 1, 3 and 6 are the most preferred transient waves. Divergent to rotational KE conversion is the most dominating mechanism for the maintenance of planetary and synoptic scale waves. All categories of waves contribute towards the maintenance of zonal flows. The primary source of energy for transient synoptic scale waves is the transient divergent rotational KE transfer whereas the interaction between zonal stationary and transient wave is likely to be secondary source. Transient KE and all transient interactions, stationary KE and all stationary interactions are found to be strongest at 500 hPa and 850 hPa respectively. Growth and decay of transient waves 1 and 3 are mainly controlled by divergent-rotational KE conversions whereas those of transient wave 6 are controlled by KE transfer due to zonal-wave interaction.With 13 Figures  相似文献   

9.
通过求取定常线性准地转位涡模式的解析解,研究了感热加热强迫所激发的副热带定常波的结构特征,讨论了基本流、牛顿冷却及地面摩擦等对定常波振幅和位相的影响。结果表明,东风时定常波在垂直方向上表现为上、下层反位相的第一斜压结构,且地面系统远强于中高层;西风时定常波呈现出向上的传播特征,在高层,随着风速增大振幅随高度的升高有增大趋势。在近地层,东风时气旋(反气旋)主体位于加热西(东)侧;西风时气旋(反气旋)主体位于加热东(西)侧,近地层以上相反。此外,发现东、西风基本流的作用具有对称特征,这与潜热加热显著不同。研究结果还表明,牛顿冷却对定常波有重要影响,基本流越弱影响越显著。在静止大气中,感热加热强迫下无斯韦尔德鲁普(Sverdrup)解,考虑牛顿冷却时,感热强迫在热源范围内的近地层和中高层分别激发出气旋式和反气旋式环流,气旋中心位于加热中心略偏西的位置。在非静止大气中,牛顿冷却项使地面系统中心向上风方向移动,东风时向东移。牛顿冷却对高、低层系统均有削弱作用。地面摩擦则明显不同,它总会使低层系统减弱,高层系统增强。  相似文献   

10.
The contribution of thermal forcing to the planetary stationary waves will be studied also by assuming that heat balance in stationary waves over zonally asymmetric thermal forcing must be maintained over a long time period. Us-ing the same model of geostrophic waves introduced in Part I, we may explain successfully the observed and simulated responses to the thermal forcing in the atmosphere, such as the wave 1 structure at high levels of middle latitudes, the seasonal changes of the stationary waves in the Northern Hemisphere, the opposite phase distributions of stationary waves at high and low levels of the subtropical regions in both hemispheres and so on.  相似文献   

11.
北半球环状模波流相互作用动力学研究进展   总被引:1,自引:0,他引:1  
梁苏洁  赵南 《气象科技》2011,39(6):753-760
总结了国内外学者对于北半球环状模(NAM:Northern Hemisphere Annular Mode)及其活动中心形成原因的研究成果。主要从NAM的天气、气候影响,波流相互作用原理对NAM形成的解释,NAM在北太平洋、北大西洋和北极3个区域活动中心的天气尺度波和行星尺度波活动等方面论述。NAM在对流层的变化与天气尺度波有关,北太平洋和北大西洋两个活动中心是天气尺度波活跃的区域,其峰值区表现为风暴轴,其中北大西洋天气尺度波破碎过程会使得NAM指数急剧变化。NAM在平流层的变化和准定常行星波关系密切,冬季准定常行星波会上传并与高纬平流层纬向流发生相互作用,从而引起北极极涡发生改变。准定常行星波将NAM 3个活动中心有机联系起来:对流层准定常行星波的纬向传播会影响北太平洋风暴轴的位置,而风暴轴的变化会影响下游北大西洋波破碎过程,同时准定常行星波的上传可以影响极涡活动。  相似文献   

12.
稳定的和不稳定的斜压行星波   总被引:1,自引:2,他引:1  
谢义炳 《气象学报》1981,39(1):44-58
本文采用两层模式,初步地应用“时空同化”的自然观,引进空间不稳定性观点,把空间不稳定性和时间不稳定性结合起来,研究振幅随纬度变化的斜压行星波的存在范围和其稳定性;得出了稳定的和不稳定的斜压行星波及其空间不稳定判据,并对传统的斜压行星波不稳定理论和判据作出鉴定,重新提出了斜压行星波时间不稳定判据,并讨论其物理含义;还得出了高层和低层斜压行星波相互强迫振动的机制以及不同纬度间扰动振幅的关系。  相似文献   

13.
本文选取行星边界层几个不同的水平温度梯度、不同的相对湿度以及地面热力分布不均匀值,用二维数值模式对一次飑线过程进行研完,其结果表明:水汽凝结潜热是对流运动发展的重要能量来源,边界层内水平温差是对流发展的重要触发条件,地面热力条件只有在有利条件配合下才可能起明显的作用。  相似文献   

14.
黄荣辉 《气象学报》1984,42(1):1-10
本文应用一个包括Rayleigh摩擦、牛顿冷却、水平涡旋热量扩散、定常、准地转、34层球坐标模式来研究冬季北半球地形与定常热源强迫所产生的定常行星波。 本文计算了强迫所产生的定常行星波引起的动量通量与热量通量。计算结果与观测结果比较一致。 计算结果表明:最大向北的动量通量与热量通量位于平流层。  相似文献   

15.
Water vapor, cloud, and surface rainfall budgets associated with the landfall of Typhoon Krosa on 6--8 October 2007 are analyzed based on a two-dimensional cloud-resolving model simulation. The model is integrated with imposed zonally-uniform vertical velocity, zonal wind, horizontal temperature, and vapor advection from NCEP/Global Data Assimilation System (GDAS) data. The simulation data that are validated with observations are examined to study physical causes associated with surface rainfall processes during the landfall. The time- and domain-mean analysis shows that when Krosa approached the eastern coast of China on 6 October, the water vapor convergence over land caused a local atmospheric moistening and a net condensation that further produced surface rainfall and an increase of cloud hydrometeor concentration. Meanwhile, latent heating was balanced by advective cooling and a local atmospheric warming. One day later, the enhancement of net condensation led to an increase of surface rainfall and a local atmospheric drying, while the water vapor convergence weakened as a result of the landfall-induced deprivation of water vapor flux. At the same time, the latent heating is mainly compensated the advective cooling. Further weakening of vapor convergence on 8 October enhanced the local atmospheric drying while the net condensation and associated surface rainfall was maintained. The latent heating is balanced by advective cooling and a local atmospheric cooling.  相似文献   

16.
夏季西风带定常扰动对东北亚阻塞高压的影响   总被引:6,自引:4,他引:6  
陆日宇  黄荣辉 《大气科学》1999,23(5):533-542
利用ECMWF 1980~1988年9年的格点资料,分析了定常扰动与东北亚阻塞高压之间的关系。分析结果表明:定常扰动的分布对阻塞高压维持日数有着重要的影响,定常扰动的季节变化可以很好地说明阻塞高压冬季多在太平洋和大西洋上发生和维持,而夏季多在东北亚地区发生和维持的特征。此外,从定常扰动的分布可以看到,不仅中高纬地区上空的正距平强度可以影响着阻塞高压的发生和维持,其南侧的负距平强度也同样重要地影响着阻塞高压。分析结果还表明:不仅定常扰动的水平结构对阻高有着重要影响,其垂直结构亦有着重要影响。最后,对夏季定常扰动进行了波数域分析,表明在夏季定常扰动的作用主要通过其中所包含的行星波、特别是行星波1波来实现,定常扰动中行星波部分的振幅变化是影响阻塞高压发生和维持的重要物理机制。  相似文献   

17.
Summary The relationships between the El-Niño phenomenon and the planetary-scale waves, and the interannual variations in the Indian monsoon (June–September) rainfall have been analysed in order to investigate how the sea surface temperature (SST) in the equatorial eastern Pacific associated with the El-Niño can produce reduced monsoon rainfall over India by teleconnections.The longitude of ridge location over the Indian region of the integrated planetary waves (numbers 1–3) along 15° N latitude circle in the height field of 200 mb pressure level in May is significantly (r=0.93, significant at 98% CL) related to the May SST anomaly at Puerto Chicama. This implies that warmer (colder) SST anomalies are associated with eastward (westward) longitude of the ridge location. The variations of the ridge location in May appear to be significantly inversely (r=–0.95, significant at 99% CL) related to the Indian monsoon rainfall, with rainfall tending to be less (more) than normal during eastward (westward) longitude of the ridge location suggesting some predictive value for the Indian monsoon rainfall. The Indian monsoon rainfall and May SST anomaly at Puerto Chicama are inversely related (r=–0.90, significant at 96% CL).In terms of the observed relationships, a plausible mechanism for linking El-Niño with the reduced Indian monsoon rainfall is discussed. The relationships noted suggest that excessive warm SST anomalies associated with El-Niño induce an eastward shift in the planetary waves which in turn reduce the Indian monsoon rainfall.With 8 Figures  相似文献   

18.
Summary The role of stationary (monthly mean) and transient (departure from monthly mean) waves within the atmospheric energy cycle is examined using global analyses from the European Centre for Medium Range Weather Forecasts (ECMWF) for the period 1980–1987. Only January and July averages are considered.It is confirmed that planetary stationary waves are basically baroclinic. Their contribution to the globally averaged energy cycle of the atmosphere is comparable to that of the transient waves. In January they contribute about 40% to the baroclinic conversion (CA) from zonal mean to eddy available potential energy. Local values for the northern hemisphere even show a predominant role of the stationary wave conversions over those originating from transient waves. Part of the available potential energy of stationary waves (A SE) is converted to kinetic energy by warm air rising and cold air sinking. Nonlinear energy conversion, which can be interpreted as destruction of stationary temperature waves by transients, is the second sink forA SE. The order of magnitude of these two processes is similar.Barotropic nonlinear conversions, though negligible in the global average, reveal large conversion rates between the mean positions of the polar and the subtropical jets. Their orientation is suggestive of a tendency to increase stationary wave kinetic energyK SE at its local minimum between the jets at the expense of the synoptic scale transients.While all terms of the energy cycle related to stationary waves reveal a predominance of the planetary scale (zonal wave numbers 1–3) transient waves are governed by synoptic scale waves (zonal wave numbers 4–9) only with respect to the baroclinic and barotropic conversions: a significant amount of transient wave energy (50% for the global average ofA TE) is due to planetary scale waves.With 15 Figures  相似文献   

19.
 We examine 800-year time series of internally generated variability in both a coupled ocean-atmosphere model where water vapor anomalies are not allowed to interact with longwave radiation and one where they are. The ENSO-like phenomenon in the experiment without water vapor feedback is drastically suppressed both in amplitude and geographic extent relative to the experiment with water vapor feedback. Surprisingly, the reduced amplitude of ENSO-related sea surface temperature anomalies in the model without water vapor feedback cannot be attributed to greater longwave damping of sea surface temperature. (Differences between the two experiments in radiative feedback due to clouds counterbalance almost perfectly the differences in radiative feedback due to water vapor.) Rather, the interaction between water vapor anomalies and longwave radiation affects the ENSO-like phenomenon through its influence on the vertical structure of radiative heating: Because of the changes in water vapor associated with it, a given warm equatorial Pacific sea surface temperature anomaly is associated with a radiative heating profile that is much more gravitationally unstable when water vapor feedback is present. The warm sea surface temperature anomaly therefore results in more convection in the experiment with water vapor feedback. The increased convection, in turn, is related to a larger westerly wind-stress anomaly, which creates a larger decrease in upwelling of cold water, thereby enhancing the magnitude of the original warm sea surface temperature anomaly. In this manner, the interaction between water vapor anomalies and longwave radiation magnifies the air-sea interactions at the heart of the ENSO phenomenon; without this interaction, the coupling between sea surface temperature and wind stress is effectively reduced, resulting in smaller amplitude ENSO episodes with a more limited geographical extent. Received: 26 March 1999 / Accepted: 25 October 1999  相似文献   

20.
准定常行星被对大气中臭氧输运的动力作用   总被引:1,自引:0,他引:1       下载免费PDF全文
本文从拉格朗日平均环流观点讨论了行星波对大气中O3。的输运作用。理论分析表明,当行星波是定常保守时,行星波对大气中O3没有输运作用;而非定常的行星被对大气中o。有明显的输运作用,它可以强迫出一个正的输运环流、即从热带上升,而从高纬下沉的环流;此外,只有当耗散的行星波传播到平流层才会在平流层强迫出输运环流。为了说明行星波对大气中O3输运的动力作用,本文还利用一组34层波-流相互耦合球坐标原始方程谱模式计算了地球大气中行星波对O3变化的作用,其计算的O3变化与实际观测到的O3分布变化很相似。  相似文献   

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