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1.
中国及周边海域对流云团的水平和垂直尺度   总被引:1,自引:0,他引:1  
利用2007年1月-2010年12月CloudSat-CALIPSO二级云产品2B-CLDCLASS-LIDAR,统计中国及其周边海域对流云的发生频率,根据对流云发生频率的分布特征将中国及周边海域划分为青藏高原(TP)、东部陆地(EC)、南部海域(SO)和西北太平洋(WP)4个子区域,并研究了4个子区域积云团和深对流云团的水平尺度和垂直尺度。统计结果表明,海洋积云团的水平尺度约为2 km,陆地积云团的水平尺度约为1 km,海洋下垫面热力性质均匀,积云团尺度更大;陆地下垫面非均匀性强,积云团分布更为零散。深对流云团的水平尺度为10-50 km,东部陆地最大,约为45 km,西北太平洋最小,约为30 km。陆地深对流云团水平尺度较海洋上大,且多尺度特征显著,应该与深对流云发生的复杂天气背景有关。积云团的垂直尺度范围为0.24-2 km,4个区域无明显差异。垂直尺度海洋深对流云团大于陆地云团,其中在南部海域地区最大,约为15 km,青藏高原最小,约为10 km。与陆地云团相比,海洋深对流云团表现为水平尺度更小、垂直尺度更大的中尺度对流体特征。   相似文献   
2.
丁治英  陈久康 《气象科学》1994,14(4):344-353
本文通过1991年梅雨后期,7月1—13日200hPa非地转场分析得出,梅雨期200hPa非地转风主要由积云对流动量转换形成。其次是风速平流,并通过数值试验得以证明。非地转风形成的高层辐散,可进一步使暴雨增强与维持。另外梅雨期非均匀层结对非地转风及暴雨也有较大的影响。  相似文献   
3.
Hydrodynamical Modeling Of Oceanic Vortices   总被引:1,自引:0,他引:1  
Mesoscale coherent vortices are numerous in the ocean.Though they possess various structures in temperature and salinity,they are all long-lived, fairly intense and mostly circular. Thephysical variable which best describes the rotation and the density anomaly associated with coherent vortices is potential vorticity. It is diagnostically related to velocity and pressure, when the vortex is stationary. Stationary vortices can be monopolar (circular or elliptical) or multipolar; their stability analysis shows thattransitions between the various stationary shapes are possible when they become unstable. But stable vortices can also undergo unsteady evolutions when perturbed by environmental effects, likelarge-scale shear or strain fields, -effect or topography. Changes in vortex shapes can also result from vortex interactions. such as the pairing, merger or vertical alignment of two vortices, which depend on their relative polarities and depths. Such interactions transfer energy and enstrophy between scales, and are essential in two-dimensional and in geostrophic turbulence. Finally, in relation with the observations, we describe a few mechanisms of vortex generation.  相似文献   
4.
A 5-level spectral AGCM (ImPKU-5LAGCM) is used to examine the sensitivity of the simulated results of the summer monsoon rainfall and circulation in East Asia to different cumulus parameterization schemes in the climatological-mean case and in the cases of weak and strong Asian summer monsoons,respectively. The results simulated with the Arakawa-Schubert's(hereafter A-S's), Kuo's and Manabe's cumulus parameterization schemes show that these simulated distributions of the summer monsoon rainfall and circulation in East Asia depend strongly on the cumulus parameterization schemes either in the climatological-mean case or in the cases of weak and strong Asian summer monsoons. From the simulated results, it might be shown that the Kuo scheme appears to be more suitable for the simulation of the summer monsoon rainfall and circulation in East Asia than the A-S scheme or the Manabe scheme, although the A-S scheme is somewhat better in the simulations of the tropical rainfall. This might be due to that the Kuo's cumulus parameterization scheme is able to reflect well the characteristics of rainfall cloud system in the East Asian summer monsoon region, where the rainfall system used to be a mixing of cumulus and stratus.  相似文献   
5.
积云对流参数化对一交梅雨锋暴雨过程影响的模拟检验   总被引:12,自引:10,他引:2  
彭新东  吴晓鸣 《高原气象》1999,18(3):451-461
应用1988年版日本谱模式JSM,对比分析了Arakawa-Sckawa-Schubert、Kain-Fritsch、KuoAnthes和Gadd-Keers等几种积云对流参数化方案在梅雨锋暴雨对流系统模拟中的表现。  相似文献   
6.
一次夏季东北冷涡中积云发展过程的数值模拟   总被引:3,自引:7,他引:3  
运用中国科学院大气物理所设计开发的三维冰雹云模式,对2002年7月11日至15日期间,发生在中国东北地区的一次由冷涡天气诱发的积云对流变化过程进行三维数值模拟。模拟结果表明:(1)冷涡诱发的积云自然降水呈中小尺度复合体的特征;(2)积云起源于低层暖湿区域里,并由强上升气流抬升到高层,得到充分发展;(3)冷涡中积云同样存在液态水累积区,一般出现在最大上升气流上,其中液态水含量随着积云的发展而变化,冰雹即在此液态水累积区0℃以下的区域内生长;(4)在模拟区域内,模拟出了多个积云单体的并合现象,而后发展为积云团;(5)模拟出的积云形态与雷达回波基本吻合。  相似文献   
7.
初始涡的结构与尺度对涡旋自组织影响的研究   总被引:5,自引:2,他引:5  
在涡旋自组织动力学的框架内,实施了9组积分时间为72 h的试验,分析初始涡廓线与初始涡尺度对多涡自组织的作用。试验的初始场上,存在着12个大小不等的β和γ中尺度的涡。若初始涡廓线为高斯型,则这些涡不能自组织形成一个α中尺度的涡;若初始涡廓线为双正弦型、抛物线型或压缩型,则这个α中尺度的涡可以形成。此外,涡廓线不同,三涡流型出现的时间迟早不一,较大尺度α中尺度涡出现的时间也迟早不一。同时,初始涡的半径大小也是影响自组织过程成败的一个重要因素。  相似文献   
8.
A diagnostie method of cumulus parameterization is suggested in which vertical transport of horizontal momentum by cumulus-scale is derived by making use of large-scale vorticity as well as divergence budget equations. Data for composite monsoon depression over India available from our earlier studies used to test the method. As a first approximation, the results are obtained using only the vorticity budget equation.The results show that in the southwest sector of the monsoon depression, which is characterized by maximum cloudiness and precipitation, there is an excess of cyclonic vorticity in the lower troposphere and anticyclonic vorticity in the upper troposphere associated with the large-scale motion. The distribution of eddy vertical transport of horizontal momentum is such that anticyclonic vorticity is generated in the lower troposphere and cyclonic vorticity aloft. Cumulus-scale eddies thus work against the large-scale system and tend to off-set the large-scale imbalance in vorticity.  相似文献   
9.
An atypical occlusion process that occurred in North China on 14 July 2011 is studied based on both observations and a real-data Weather Research and Forecasting (WRF) model simulation. The results show that this atypical occlusion process was significantly different from the traditional, synoptic-scale occlusion process that occurs within extratropical cyclones. It was caused by the merger of two cold-type mesoscale fronts. One of the fronts developed from the gust front of convective storms, while the other was a sea-breeze front. As the two fronts moved towards each other, the warm air between them was squeezed and separated from the surface. An atypical occluded front was formed when the two fronts merged, with the warm air forced aloft. This kind of occlusion is termed a "merger" process, different from the well-known "catch-up" and "wrap-up" processes. Moreover, local convection was found to be enhanced during the merger process, with severe convective weather produced in the merger area.  相似文献   
10.
A new method to detect and study young star clusters is presented. This is based on the knowledge that the light of stellar populations with ages between ∼ 200 Myr and ∼ 1/2 Gyr is dominated by very red, bright AGB stars. Star clusters undergoing this so-called ‘AGB phase transition’ are featured by very red V-K colours, like those of Magellanic Clouds clusters, while optical colours like B-V remain blue typical for young populations. The best channel for detecting star clusters in this age range is therefore the near IR. From the theoretical side, SSP models including properly the contribution of the bright AGB are required (Maraston, 1998). Using this strategy, we succesfully detected the AGB phase transition among the clusters of the merger remnant galaxy NGC 7252 (see Maraston etal., 2001). This revised version was published online in September 2006 with corrections to the Cover Date.  相似文献   
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