华南后汛期降雨量的振动和分布   总被引：8，自引：0，他引：8  

何有海  关翠华  林锡贵  金祖辉 《热带气象学报》1998,14(4):359-363

对１９５９至１９８８年华南后汛期（７－９月）降雨量距平百分率的大尺度变化特征进行了分析,并与前汛期（４－６月）降雨量的情况进行了比较,同时探讨了后汛期降雨量异常的成因。结果表明,华南后汛期雨量存在明显的年际变化,且地区差异显著;后汛期降雨量的异常与热带西太平洋的海水温度、南海地区大气的对流活动及登陆我国东南沿海地区的热带气旋的频数有关。  相似文献   

太阳5分钟振荡的激发机制     

熊大闰  邓李才 《天文学报》2009,50(4)

1 引言 太阳5分钟振荡是上世纪1个重要的发现[1],它使得人们可以通过观测太阳表面的振动来探测其内部的结构,日震学已取得了巨大的进展,然而我们至今仍不了解其脉动的激发机制,它依然是1个存在争议的问题.太阳位于造父变星脉动不稳定区之外,所以大多数人都相信,由于对流的阻尼,太阳是脉动稳定的,太阳和太阳型恒星的振荡都是由所谓的湍流随机激发机制所激发[2-8].  相似文献   

On the propagation of topographically trapped waves     

Stefano Pierini 《地球物理与天体物理流体动力学》2013,107(1-4):97-108

Abstract

In the context of ageostrophic theory in a homogeneous ocean, a nondimensional number is determined which corresponds to the Ursell number for long gravity waves. It is defined as Q = NL ²/h ³, where N is the amplitude of the wave travelling along the long length-scale direction, L is its length and h (which for gravity waves is the water depth) is given by h=(l ⁴ f ²/g)^1/3. where l is the short length-scale, f the Coriolis parameter and g the acceleration due to gravity. The physical meaning of Q is as follows: if Q? O(1) the free evolution of the wave is linear and weakly dispersive, if Q = O(1) nonlinear and dispersive effects balance out and finally if Q ?O(1) the evolution is nonlinear and non-dispersive. Expressions for the time scales for the development of dispersive and nonlinear effects are also determined. These results apply to topographically trapped waves, namely barotropic continental shelf and double Kelvin waves travelling along a rectilinear topographic variation.  相似文献   

Finite amplitude convection and magnetic field generation in a rotating spherical shell     

Ke-Ke Zhang  F. H. Busse 《地球物理与天体物理流体动力学》2013,107(1-4):33-53

Abstract

Finite amplitude solutions for convection in a rotating spherical fluid shell with a radius ratio of η=0.4 are obtained numerically by the Galerkin method. The case of the azimuthal wavenumber m=2 is emphasized, but solutions with m=4 are also considered. The pronounced distinction between different modes at low Prandtl numbers found in a preceding linear analysis (Zhang and Busse, 1987) is also found with respect to nonlinear properties. Only the positive-ω-mode exhibits subcritical finite amplitude convection. The stability of the stationary drifting solutions with respect to hydrodynamic disturbances is analyzed and regions of stability are presented. A major part of the paper is concerned with the growth of magnetic disturbances. The critical magnetic Prandtl number for the onset of dynamo action has been determined as function of the Rayleigh and Taylor numbers for the Prandtl numbers P=0.1 and P=1.0. Stationary and oscillatory dynamos with both, dipolar and quadrupolar, symmetries are close competitors in the parameter space of the problem.  相似文献   

Large wavenumber convection in the rotating annulus     

A. Abdulrahman  C. A. Jones  M. R. E. Proctor  K. Julien 《地球物理与天体物理流体动力学》2013,107(3-4):227-252

Abstract

The annulus model considers convection between concentric cylinders with sloping endwalls. It is used as a simplified model of convection in a rapidly rotating sphere. Large azimuthal wavenumbers are preferred in this problem, and this has been exploited to develop an asymptotic approach to nonlinear convection in the annulus. The problem is further reduced because the Taylor-Proudman constraint simplifies the dependence in the direction of the rotation vector, so that a nonlinear system dependent only on the radial variable and time results. As Rayleigh number is increased a sequence of bifurcations is found, from steady solutions to periodic solutions and 2-tori, typically ending in chaotic behaviour. Both the magnetic (MHD convection) and non-magnetic problem has been considered, and in the non-magnetic case our bifurcation sequence can be compared with those found by previous two-dimensional numerical simulations.  相似文献   

水汽和潜热释放对背风波影响的数值试验          下载免费PDF全文

臧增亮  潘晓滨  汪潮  王劲 《气象科学》2012,32(1):38-44

利用中尺度数值模式ARPS进行了理想场的数值模拟,分析研究了水汽和潜热释放对大气层结稳定度的影响以及其在背风波的发展和演变过程中的作用,研究发现,潜热释放对大气层结分布的影响要远大于水汽对大气层结分布的直接影响,如果没有潜热的释放,水汽对背风波的发展和演变的作用非常小,而潜热释放可以使湿层结稳定度急剧下降,迅速破坏原有的层结分布,使这个区域出现非拦截的强烈的垂直运动,波动的崩溃更加迅速和明显。但需要说明的是在试验中,将数值模式里控制潜热释放的参数设为:0、1/2、2的假定情况,则在实际的大气运动过程中是不可能存在的。  相似文献   

1—3月北极涛动对北半球热带太平洋和大西洋对流活动的可能影响   总被引：1，自引：0，他引：1  

胡淼  龚道溢  王璐  周天军  张自银 《气象学报》2012,70(3):479-491

利用1979—2008年日分辨率的向外长波辐射资料以及NCEP再分析资料,去除ENSO影响后,分析了1—3月北极涛动对热带太平洋和热带大西洋对流活动及降水的可能影响。结果表明北极涛动偏强(弱)时,热带太平洋和大西洋对流活动显著偏强(弱)。北半球热带大洋冬季平均向外长波辐射与北极涛动指数的相关系数存在两个显著负相关区:一个位于中太平洋区,大致包括13°—20°N、160°E—170°W;另外一个位于热带大西洋,显著区覆盖的范围大体包括5°—20°N、15°—70°W。这些区域的降水量也表现出显著的正相关。向外长波辐射、强对流面积指数、强对流强度指数、平均降水量等指标与北极涛动指数的相关均以冬季同期最高,随时间滞后相关迅速减弱。与此对应的对流层低层大气环流也有显著变化,850hPa风场的变化表现为热带太平洋有异常的气旋性环流,气旋中心区与显著强对流和降水异常区一致。而热带大西洋有显著的经向环流辐合和风切变,与异常对流和降水区吻合。海洋模式的模拟结果表明,与北极涛动有关联的海温分布,很大程度上与大气强迫有关,说明热带1—3月降水和对流活动与海温的关联较弱。北极涛动与热带太平洋、大西洋对流和降水活动之间主要是通过大气环流的变动产生联系的。  相似文献   

伊犁一次区域性暴雨分析     

祝小梅 《沙漠与绿洲气象(新疆气象)》2012,6(2):49-52

利用伊宁新一代天气雷达资料,结合高空和地面观测资料,分析了2010年7月19日伊犁地区一次局地暴雨天气过程。结果表明：此次强对流天气过程的主要影响系统为500 hPa中亚低槽、200hpa高空急流、低层风速辐合和地面雷暴高压。较强的层结不稳定和低层垂直风切变有利于对流的产生;云图和雷达资料分析表明,此次局地暴雨是由中尺度强对流云团产生,具有典型的对流单体形成、发展成回波短带合并形成带状回波,该带状回波最后演变成一个尺度较大的弓形回波。  相似文献   

高原涡诱生西南涡特大暴雨成因的个例研究   总被引：25，自引：6，他引：19       下载免费PDF全文

赵玉春  王叶红 《高原气象》2010,29(4):819-831

利用多途径探测与再分析资料,通过诊断分析、数值模拟和敏感性试验,对2008年7月20～21日一次高原涡东移诱生西南涡并引发川中特大暴雨的天气过程进行了初步分析,探讨了西南涡特大暴雨发生的中尺度环境场特征,特殊地形和非绝热物理过程在高原涡东移诱生西南涡特大暴雨中的作用。结果表明,高原涡形成后沿高原东北侧下滑,在四川盆地诱生出西南涡,川中特大暴雨在西南涡形成过程中由强中尺度对流系统(MCSs)的活动造成。高原涡东移诱生的低层偏东气流在川西高原东侧地形的动力强迫抬升作用下,释放对流有效位能激发出MCSs产生强降水,降水凝结潜热加热反馈驱动西南涡快速发展。地形的动力作用仅能形成浅薄的西南涡,降水凝结潜热的加入才能使西南涡充分发展。高原涡的发展主要受地面热通量影响,它的发展与否在很大程度上决定西南涡能否形成。盆地周边高大山脉对西南涡的位置分别有不同程度的影响,而盆地周边高大山脉上叠加的中小尺度地形对西南涡和暴雨带的整体位置影响不大,在一定程度上影响暴雨的落区。  相似文献   

Adaptation of Pressure Based CFD Solvers for Mesoscale Atmospheric Problems   总被引：1，自引：1，他引：0  

Gergely Kristóf  Norbert Rácz  Miklós Balogh 《Boundary-Layer Meteorology》2009,131(1):85-103

General purpose Computational Fluid Dynamics (CFD) solvers are frequently used in small-scale urban pollution dispersion simulations without a large extent of ver- tical flow. Vertical flow, however, plays an important role in the formation of local breezes, such as urban heat island induced breezes that have great significance in the ventilation of large cities. The effects of atmospheric stratification, anelasticity and Coriolis force must be taken into account in such simulations. We introduce a general method for adapting pressure based CFD solvers to atmospheric flow simulations in order to take advantage of their high flexibility in geometrical modelling and meshing. Compressibility and thermal stratification effects are taken into account by utilizing a novel system of transformations of the field variables and by adding consequential source terms to the model equations of incompressible flow. Phenomena involving mesoscale to microscale coupled effects can be analyzed without model nesting, applying only local grid refinement of an arbitrary level. Elements of the method are validated against an analytical solution, results of a reference calculation, and a laboratory scale urban heat island circulation experiment. The new approach can be applied with benefits to several areas of application. Inclusion of the moisture transport phenomena and the surface energy balance are important further steps towards the practical application of the method.  相似文献