江淮梅雨对东亚副热带夏季风进程及海温异常的响应

利用1960—2020年江淮地区75个气象站逐日降水量、气温、相对湿度资料以及NCEP/NCAR再分析资料和Hadley中心海表温度资料，研究了东亚副热带夏季风进程变异对江淮梅雨的影响，揭示了不同类型梅雨期太平洋海温及大气环流异常特征。结果表明：8种江淮梅雨类型中，多雨型占45.9%，少雨型占54.1%，其中多雨型在前30 a占36.7%，后31 a占63.3%。江淮典型梅雨年（高温高湿多雨）的主要特征为安徽南部、江苏中部及湖北东部地区降水偏多，安徽南部、江西东北部及浙江西北部气温偏高，淮河流域湿度大；而在非典型梅雨年（低温低湿少雨）大部分地区雨量偏少，气温呈"东高西低"分布，低温中心区位于淮河中游，湿度呈"西大东小"分布。欧亚大陆中高纬度阻塞高压增强，脊前向南输送的西北气流加强且路径偏东，中国东北冷涡强度较强且位置偏西南，东亚大槽加深，槽后冷空气向南输送，有利于典型梅雨形成。当前期冬春季赤道东太平洋海温异常偏高，西太平洋海温异常偏低时，西太平洋副热带高压强度偏强、面积偏大、脊线位置偏南、西伸脊点偏西，东亚副热带夏季风推进到江淮地区的时间偏早，出梅偏晚，梅雨期降水量偏多。     

人口密度的空间连续分布模型

分析了常用的表示人口分布的方法,并指出了其不足的地方,提出了模拟人口空间分布的必要性,同时提出了模拟人口空间分布的思路。将研究区域划分为一定分辨率的格网,用核心估计方法将人口密度估计值分配到每个格网上,每个格网上的人口是均匀分布的,随着格网分辨率的提高,就可以模拟出符合人口详细分布的人口密度空间连续分布模型,并通过实验说明该方法是可行的。     

Vertical Structure in the Marine Atmospheric Boundary Layer and its Implication for the Inertial Dissipation Method

The structure of the marine atmospheric boundarylayer and the validity ofMonin–Obukhov similarity theory over the seahave been investigated using longterm measurements. Three levels of turbulencemeasurements (at 10 m, 18 mand 26 m) at Östergarnsholm in themiddle of the Baltic Sea have beenanalysed. The results show that turbulentparameters have a strong dependenceon the actual height due to wave influence.The wind profile and thus thenormalised wind gradient are very sensitiveto wave state. The lower part of theboundary layer can be divided into three heightlayers, a wave influenced layerclose to the surface, a transition layer andan undisturbed ordinary surfacelayer; the depth of the layers is determinedby the wave state. This heightstructure can, however, not be found for thenormalised dissipation, which is onlya function of the stability, except duringpronounced swell where the actualheight also has to be accounted for. Theresults have implications for the heightvariation of the turbulent kinetic energy(TKE) budget. Thus, the imbalancebetween production and dissipation willalso vary with height according to thevariation of wave state. This, in turn,will of course have strong implicationsfor the inertial dissipation method, inwhich a parameterisation of the TKEbudget is used.     

"98.7"特大暴雨低涡的螺旋度和动能诊断分析

“98．7”特大暴雨过程与700hPa低涡切变线的强烈发展以及丰沛的水汽和强垂直运动密切相关。螺旋度的诊断结果揭示,与强暴雨区和切变线低涡相应的是一对符号相反而又紧邻的螺旋度带。它们的垂直结构是一对符号相反而又互伴的螺旋度柱;螺旋度及其诸分量的量级是相同的。这表明,垂直运动的水平切变和水平速度的垂直切变以及水平速度的水平切变对螺旋度有相同大小的员献,也意味着强垂直运动和低空急流对暴雨的发生和发展极其重要。动能的诊断结果显示。强动能区与暴雨区和低涡切变线有很好的对应关系,在中、低空的强动能中心也正是强降雨中心;动能最强的700hPa也是低涡切变线发展最强的层面。强动能及其强梯度区和强螺旋度区基本一致。表明强动能及其强梯度对螺旋度变率及其通量有重要贡献。     

新疆伽师强震群强震主破裂面走向初探

1997年1月21日-1998年8月27日新疆伽师发生了包含9次6级地震的强震群,震源机制解表明有NE向和NW向两个节面．有观点认为主破裂面为NNW向．本通过数字地震台阵的余震序列精确定位、震源破裂过程及滑动方向、震群空间分布图像、地震烈度等震线长轴走向和微、宏观震中动态变化方向等多种方法分析后,综合判定9次6级地震的主破裂面走向极可能为北东方向．     

A remote sensing model for monitoring soil evaporation based on differential thermal inertia and its validation

To develop geosciences quantification and multi-dimensional researches will be an inevitable trend in the 21st century. The interaction between the land surface and the atmosphere not only serves as an important component in geosciences quantification, bu…     

Sea surface height and transport stream function of the South China Sea from a variable-grid global ocean circulation model

The study on the South China Sea (SCS) circulation has a history of more than 40 years. Nevertheless, the SCS circulation is not fully understood compared with the Bohai Sea, Yellow Sea and East China Sea (ECS). Many numerical studies on the SCS circulati…     

A consistent derivation of the wave-energy equation from basic hydrodynamic principles

Based on a decomposition of the velocity into mean flow, turbulent and wave components, momentum and hereafter a wave-energy equation is derived. It contains a turbulent energy dissipation term which is closed by applying a wave-related mixing length model and linear wave theory solutions. This closure produces a non-linear turbulent wave-energy dissipation including the wave energy in a 5/2 power law. The theory is able to predict correctly the shape of deep-water wave spectra according to Phillips' similarity law.Responsible Editor: Hans Burchard     

The system of the Milky Way, LMC and SMC

A simple sticky-particle numerical model has been developed in order to check whether extended structures of gas created due to the dynamical evolution of the Galaxy and the Magellanic Clouds system can be explained as remnants of a tidal interaction. Influence of dissipative nature of gaseous medium has been taken into account. The most remarkable features are: the Magellanic Stream, the common HI envelope surrounding both the LMC and SMC and the bridge extended between the Clouds. In contrast to previous works of Murai and Fujimoto (1980), Gardiner et al. (1994) and H and Rohlfs (1994) no presumptions were done on the actual galactocentric velocities of the Magellanic Clouds. The mean values of the LMC and SMC velocity vectors obtained from the Hipparcos proper motion measurements (Kroupa and Bastian, 1997) were used in order to verify whether they allow to reproduce the observed HI distribution. Numerical simulations showed that tidal forces are really significant for the evolution of extended structures such as the Magellanic Stream but this approach becomes unsufficient for the internal regions of galaxies where self-gravity and dissipative properties of the gas cannot be neglected. More precise proper motion measurements are urgently needed. This revised version was published online in August 2006 with corrections to the Cover Date.     

An Origin for the Linear Magnetic Anomalies on Mars through Accretion of Terranes: Implications for Dynamo Timing

The proposed existence of magnetic lineations in the Terra Cimmeria and Terra Sirenum regions of Mars was initially explained by Earth-like sea-floor spreading. Here we argue instead that these lineations could have been formed at a convergent plate margin through collision and accretion of terranes. A similar process produced banded magnetic anomalies, similar in geometry and even in size to those in Earth's North American Cordillera. Because only sparse and generally weak anomalies have been detected in the martian northern lowlands, which could constitute an analog to the terrestrial oceanic crust, it is possible that the magnetic field stopped its activity while crustal recycling was still active in Mars.