三亚湾海岸动力演变的数值模拟研究

近年来,海岸侵蚀呈现不断加剧的趋势,给沿海地区经济社会的发展造成了极大危害。关于三亚湾海岸侵蚀过程及其动力学研究多停留在定性或半定量阶段。从海岸动力地貌学角度出发,基于沉积物迁移理论,利用数值模拟方法,定量研究了三亚湾海岸在波浪和潮流作用下的动力演变过程。计算结果重现了海水波浪的传播形态及动态特征:涨潮时,波高极值相对较大,水位随之升高,波动现象明显,波动形态复杂;落潮时,波高极值相对减小,水位也随之降低,海面相对较平静,波形态在离岸区域较单一,仅在近岸区域相对多样化。同时,数值模拟结果也很好地显示了三亚湾岸线附近的沉积或侵蚀过程特征:三亚湾西段海洋动力条件较强,沉积或侵蚀现象明显,沉积/侵蚀能力由三亚湾西段逐渐向东段减小。此外,以海洋动力学机制为基础,定量模拟了三亚湾海岸侵蚀与演变物理过程,为该地区海岸开发利用、海岸环境保护提供科学依据。     

梨树断陷断陷期小宽断裂带构造应力场数值模拟

在小宽断裂带构造解析基础之上,根据地质资料以及前人提供的岩石物理学参数建立了梨树断陷区的二维地质和数值模型。进行了构造应力场数值模拟,分析了梨树断陷小宽断裂带断陷期小宽断裂带断陷期在沙河子期(K1sh)、营城期(K1yc)、登楼库期(K1d)的构造应力场特征。模拟结果显示：(1)沙河子期在左旋走滑应力状态下,小宽断裂带处于近NE—SW方向的拉张应力状态,剪应力在沿着断裂带SW—NE走向逐渐减小; (2)营城期在右旋走滑的应力状态下,小宽断裂带处于近NW—SE向的拉张力状态,剪应力最大值位于断裂带的最中间部位;(3)登楼库期在左旋走滑的应力状态下,断裂带处于SWW—NEE向的张拉应力状态,剪应力最大值位于断裂带西南段。     

NUMERICAL SIMULATION OF OZONE DISTRIBUTIONS AND ITS VARIATION MECHANISM*

A 2-D global chemistry-transport model is set up in this paper.The model simulates the atmospheric ozone distributions well with specified dynamical conditions.The analysis of ozone variation mechanism shows that ozone is chemically in quasi-equilibrium except for the polar night region where the variation of ozone concentration is under the control of dynamical processes,that the oxygen atoms which produce ozone are mainly provided by the photolysis of O₂ in the upper stratosphere and by the photolysis of NO₂ in the lower stratosphere and the troposphere.and that the ozone is destroyed mainly by NO_x:the reactions between NO_x and O₃ and the odd oxygen cycle contribute 80% to more than 90% of the ozone destruction.     

渤、黄、东海内潮的数值模拟

在全球的海洋中,中国东海和临近海域是最显著的内潮生成地之一。本文采用NODC(Levitus) World Ocean Atlas 1998提供的季平均温、盐资料,计算海水的密度,并计算垂向密度梯度的最大值点,得到一个较符合海水实际的密度分层。使用三维非线性数值模型(将海洋分为2层)研究了潮汐(M2,S2,K1,O1分潮)作用下渤黄东海的内潮,揭示了整个海区内潮起伏的空间分布,结果发现大振幅的波动均发生在台湾东北(冲绳海槽)海域和中国近海地形突变之处,其中前者更显著。对于各分潮模拟得到的表面潮与TOPEX/Poseidon高度计资料基本一致。研究结果表明上层海水的深度和厚度的梯度对内潮有一定的影响;冬季分布区域比夏季小,强度比夏季大。     

Experimental Investigation and Numerical Analysis to Develop Low-Energy Large-Midwater Trawls

Fuel consumption in fisheries is a primary concern because of its effects on the environment and the costs incurred by fishermen. Many studies have been conducted to reduce the fuel consumption in fishing operations. Fuel consumption due to fishing gear during a fishing operation is generally related to the hydrodynamic resistance on the gear. This means that fuel consumption is proportional to the drag created by the towing speed. Based on numerical methods, this study suggests a new approach to reduce fuel consumption in fisheries. The results of the simulation are in good agreement with those of model experiments. The total as well as partial resistance forces on the gear are calculated by simulation. The simulation results suggest improved materials and gear structure for reducing the hydrodynamic forces on the gear while maintaining gear performance. The method for assessing the gear performance involves measuring the height and width of the net mouth. Furthermore, this study investigates the efficiency of a low-energy trawl from an economic point of view. The findings of this study will be useful in reducing greenhouse gas (GHG) emissions in fishing operations, and thereby contribute toward lowering fishing costs by saving fuel.     

非饱和土三轴压缩应力路径试验的数值模拟研究

应力路径对土的强度和变形性质具有重要影响。相对于饱和土而言,控制吸力条件下的非饱和土三轴压缩状态的应力路径研究更加复杂。随着非饱和土本构理论的不断发展,理论和试验研究结果表明,非饱和土弹塑性本构模型可以用来近似地描述非饱和土的强度和变形性质。因而,运用非饱和土弹塑性本构模型对控制吸力条件下的3种非饱和土三轴压缩应力路径试验进行数值模拟是一种有效的理论研究手段。采用Barcelona模型能够对此类试验进行较好的数值模拟,其研究结果表明,在控制吸力条件的三轴压缩状态下应力路径对非饱和土的强度和变形性质具有重要影响。     

The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering

We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of magnitude larger than previous redshift surveys used to address this issue. We measure the projected two-point correlation function of galaxies in a series of volume-limited samples. The projected correlation function is free from any distortion of the clustering pattern induced by peculiar motions and is well described by a power law in pair separation over the range     . The clustering of     galaxies in real space is well-fitted by a correlation length     and power-law slope     . The clustering amplitude increases slowly with absolute magnitude for galaxies fainter than M *, but rises more strongly at higher luminosities. At low luminosities, our results agree with measurements from the Southern Sky Redshift Survey 2 by Benoist et al. However, we find a weaker dependence of clustering strength on luminosity at the highest luminosities. The correlation function amplitude increases by a factor of 4.0 between     and −22.5, and the most luminous galaxies are 3.0 times more strongly clustered than L * galaxies. The power-law slope of the correlation function shows remarkably little variation for samples spanning a factor of 20 in luminosity. Our measurements are in very good agreement with the predictions of the hierarchical galaxy formation models of Benson et al.     

日本琵琶湖表面定振波的计算

利用水动力学方程对口本琵琶湖表面定振波进行了计算和分析,结果表明其主要周期约为69．5min,另外,利用实测水位资料,采用最大熵谱法进行分析,得到了主要周期约为68min,两者吻合很好。     

宁夏区域精细化温度预报业务平台

介绍以宁夏中尺度数值模式温度预报为基础,以宁夏精细化预报系统温度预报产品为核心,结合自动气象站等多种资料,以图形方式显示、修改和制作宁夏各站逐时温度预报业务平台。该平台以宁夏各地区代表站与该地区其它站之间的回归方程的计算量为依据,在温度预报物理过程不变的情况下,通过修改曲线的方式,完成对大数据量温度预报值的订正。该平台的建成,为制作高时间密度的预报提供了技术支撑。     

裸眼井中软地层多极子源激发的弹性波的传播

利用全波场和分波场算法对裸眼井软地层中由单极子源和多极子源（偶极子源和四极子源）激发的弹性波进行了数值研究,给出了声波全波列理论波形、纯纵波和纯横渡理论波形及纵横波的频率传输特性曲线.结果表明,纯纵波和纯横波是无频散几何衰减波;除了在vs>（1-ρ1/ρ2）1/2v1的井眼中由单极子源激发的横波无传播特征频率外,纵横波都具有各自的传播特征频率,纵波的传播特征频率有一系列离散值,横波的传播特征频率只有一个且等于非对称模式波的截止频率;多极子源激发的纵波传播特征频率的最小值大于横波的传播特征频率,随着极子数增多,二者的特征频率值皆增高,差别也越大,因此,当声源发射主频较低,接近横波传播特征频率而远离纵波传播特征频率时,低频多极子源将压制纵波并激发出较强的横波,分析结果还表明,通常所说的低频多极子源激发出的横波波群实际上是纯横波与截止频率附近的非对称模式波叠加的结果,在其它条件不变时,二老对横波波群相对贡献的大小取决于声源激发主频的高低及其带宽的大小.