Numerical simulation and synoptic analysis of dust emission and transport in East Asia

This study is concerned with the mechanisms of dust storm development in East Asia and the characteristics of the responsible synoptic systems. Two severe East Asian dust storms which occurred in spring 2002 are analyzed using synoptic and remote sensing data. The relationships between the formation and the movement of the dust storms and the evolution of the synoptic systems are examined. It is shown that a dust storm may develop when a synoptic system moves to the desert area of Northeast Asia with a surface wind speed exceeding 6 m s^− 1. Numerical simulations of the two dust storms are carried out using a dust storm forecasting model. The performance of the model is verified with observations. The dust sources are found to be consistent with the desert regions in Northeast Asia, but cover a somewhat larger area than the observations suggest. Finally, we present a conceptual model of dust storm generation and movement in East Asia on the basis of numerical modeling and synoptic analysis.     

A numerical study of daily transitions in the convective boundary layer

We examine daily (morning–afternoon) transitions in the atmospheric boundary layer based on large-eddy simulations. Under consideration are the effects of the stratification at the top of the mixed layer and of the wind shear. The results describe the transitory behaviour of temperature and wind velocity, their second moments, the boundary-layer height Z _m (defined by the maximum of the potential temperature gradient) and its standard deviation σ _m , the mixed-layer height z _i (defined by the minimum of the potential temperature flux), entrainment velocity W _e, and the entrainment flux H _i . The entrainment flux and the entrainment velocity are found to lag slightly in time with respect to the surface temperature flux. The simulations imply that the atmospheric values of velocity variances, measured at various instants during the daytime, and normalized in terms of the actual convective scale w_*, are not expected to collapse to a single curve, but to produce a significant scatter of observational points. The measured values of the temperature variance, normalized in terms of the actual convective scale Θ_*, are expected to form a single curve in the mixed layer, and to exhibit a considerable scatter in the interfacial layer.     

湿静力平衡温度及其在大气对流运动中的应用

提出了一个新的大气动力-热力学温湿参量——湿静力平衡温度（T_s）。它与密度温度（T_ρ）有密切关系。作为T_s的应用示例,简化了积云一维时变模式垂直运动方程;提出了“载水气块”和“非载水气块”统一的新的“对流有效位能”表达式。结合实例,计算了“载水气块”和“非载水气块”两种情况下的对流有效位能（分别记作CAPE_w和CAPE）以及对流抑制能量（分别记作CIN_w和CIN）等,“载水气块”与“非载水气块”两种情况的“对流有效位能”及“对流抑制能量”有较大差异。作为强对流天气分析预报的重要参数,目前计算对流有效位能和对流抑制能量的通用公式存在一定缺陷;在对“对流有效位能”的理解方面存在某些模糊认识和盲点。从新的观察角度对“对流有效位能”的概念做了详细分析并进一步阐明了其确切含义。新的方案同样可以方便地在T-lnp图上进行稳定度分析,并可根据新的公式对T-lnp的某些缺点进行修正。     

对流温度含义阐释及部分示意图隐含悖论成因分析与预报应用

分析和预报局地对流时常用到对流温度,对流凝结高度常被用于估计局地对流云的云底高度。对流温度和对流凝结高度用于局地对流分析时存在一定的前提,且其蕴含的物理意义非常丰富。论文剖析了几本较为经典的气象专业书籍中对流温度概念图示,指出其中隐含的悖论,包括与大气稳定度基本常识相悖、违反大气能量学理论、以及与物理量本身含义明显抵触。进一步阐释构图不够严谨、对对流温度含义理解不完全到位是出现这种悖论的根本原因。并构造了物理意义清晰、气象基本理论更为合理的对流温度示意图。利用观测资料,分析了北京夏季对流云的发生频数和生成时间,尝试用对流温度预报局地对流云的生成,用对流凝结高度预报局地对流云云底高度。结果表明,对流温度在局地对流云的预报中具有一定的指示意义,对流凝结高度能在一定程度上反映出局地对流云的云底高度。如果将最高温度不低于对流温度1℃作为判定能否产生对流云的一个标准,临界成功指数达到45%。     

减弱对流云降水的AgI催化原理的数值模拟研究

在对流云模式中增加了AgI两个预报量,耦合了考虑受水汽过饱度和温度影响的4种核化机制的AgI催化模块,使其具备了对AgI类催化剂的模拟能力,能够研究AgI类催化剂对对流云系统的影响。利用该模式对一次华南对流云降水过程进行了AgI催化数值模拟试验,对人工减缓对流云降水的可能性及原理进行了研究。模拟结果表明,在适当的时机对适当的部位进行大剂量的催化,可以减少总降水量,也可以减少最大降水中心的雨强。当催化浓度达到2×10~8 kg~(-1)时,可以减少32%的降水量,具备有效减缓对流云降水的可能性。大剂量催化后,大量的AgI粒子在冷区核化后,消耗了大量的过冷水。催化后霰粒子的落速和雨水的落速减小。催化阶段由于霰融化成雨水减少而使降水减弱。催化结束后在霰融化成雨水增多的情况下,雨水的蒸发大幅增加,从而导致了降水量的持续减少。AgI在模拟的强对流云中主要以受过饱和度影响的凝结冻结和催化剂长时间作用的浸没冻结这两种方式成核。研究所用催化方法在外场作业中具有技术可行性。     

BUILDING DENSITY AND INTERIOR BUILDING TEMPERATURES: A PHYSICAL MODELING EXPERIMENT

The effect of building density on the interior temperatures of buildings is explored using scaled physical models. The urban canopy layer is modeled as a single-cube structure surrounded by a wall that represents neighboring structures. Each physical model was constructed of plywood and consisted of a cube 200 mm in height, enclosed by a wall 200 mm in height. Four models were constructed corresponding to height/width ratios (H/W) of 4, 2, 1, and 0.5 and placed at an exposed site located at 34°N. The interior air temperature of each cube, direct and diffuse solar radiation on a horizontal surface, and ambient air temperature and wind velocity were measured over a period from late November 1996 to early June 1997. To extract the influence of building density, air temperatures were compared against those measured in the model representing a H/W of 1. The results show that nighttime cooling is primarily a function of building density, but that daytime heating depends on the interaction of density with changing model-sun relationships. [Key words: urban canopy layer, building air temperature, building density, physical model.]     

Dynamics of convective dissolution from a migrating current of carbon dioxide

During geologic storage of carbon dioxide (CO₂), trapping of the buoyant CO₂ after injection is essential in order to minimize the risk of leakage into shallower formations through a fracture or abandoned well. Models for the subsurface behavior of the CO₂ are useful for the design, implementation, and long-term monitoring of injection sites, but traditional reservoir-simulation tools are currently unable to resolve the impact of small-scale trapping processes on fluid flow at the scale of a geologic basin. Here, we study the impact of solubility trapping from convective dissolution on the up-dip migration of a buoyant gravity current in a sloping aquifer. To do so, we conduct high-resolution numerical simulations of the gravity current that forms from a pair of miscible analogue fluids. Our simulations fully resolve the dense, sinking fingers that drive the convective dissolution process. We analyze the dynamics of the dissolution flux along the moving CO₂–brine interface, including its decay as dissolved buoyant fluid accumulates beneath the buoyant current. We show that the dynamics of the dissolution flux and the macroscopic features of the migrating current can be captured with an upscaled sharp-interface model.     

暴时内辐射带高能质子的损失和恢复机制探究

我们利用NOAA17卫星对内辐射带高能质子的观测结果研究了大磁暴期间内辐射带质子通量的变化过程.我们发现内辐射带质子出现两种不同的暴时损失事件.在大磁暴发生时,内辐射带外边界质子通量会迅速减小,然后缓慢恢复;而在内辐射带中心区的质子通量(即南大西洋异常区(SAA)质子通量最大值)的暴时变化表现为质子通量的一个迅速的减小和迅速恢复.内辐射带外边界的损失事件主要发生在较低能量质子能档,而内辐射带中心处的损失事件发生在所有质子能档.两种损失事件中质子通量的不同变化意味着内辐射带质子可能有不同的损失和产生机制.通过分析,我们认为内辐射带外边界处质子通量损失事件主要由磁场曲率散射机制造成,而其恢复机制主要是宇宙线反照中子衰变(CRAND).内辐射带中心区(即南大西洋异常区质子通量最大处)质子通量损失事件可能与Dst效应有关.     

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Beach erosion and recovery during consecutive storms at a steep‐sloping,meso‐tidal beach

This study analyses beach morphological change during six consecutive storms acting on the meso‐tidal Faro Beach (south Portugal) between 15 December 2009 and 7 January 2010. Morphological change of the sub‐aerial beach profile was monitored through frequent topographic surveys across 11 transects. Measurements of the surf/swash zone dimensions, nearshore bar dynamics, and wave run‐up were extracted from time averaged and timestack coastal images, and wave and tidal data were obtained from offshore stations. All the information combined suggests that during consecutive storm events, the antecedent morphological state can initially be the dominant controlling factor of beach response; while the hydrodynamic forcing, and especially the tide and surge levels, become more important during the later stages of a storm period. The dataset also reveals the dynamic nature of steep‐sloping beaches, since sub‐aerial beach volume reductions up to 30 m³/m were followed by intertidal area recovery (–2 < z < 3 m) with rates reaching ~10 m³/m. However, the observed cumulative dune erosion and profile pivoting imply that storms, even of regular intensity, can have a dramatic impact when they occur in groups. Nearshore bars seemed to respond to temporal scales more related to storm sequences than to individual events. The formation of a prominent crescentic offshore bar at ~200 m from the shoreline appeared to reverse the previous offshore migration trend of the inner bar, which was gradually shifted close to the seaward swash zone boundary. The partially understood nearshore bar processes appeared to be critical for storm wave attenuation in the surf zone; and were considered mainly responsible for the poor interpretation of the observed beach behaviour on the grounds of standard, non‐dimensional, morphological parameters. Copyright © 2011 John Wiley & Sons, Ltd.