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81.
The viscosity of a synthetic andesite-like melt was measured in the low viscosity range (101-106 Pa s) using the falling sphere(s) method and in the high viscosity range (108-1013 Pa s) using parallel-plate viscometry. Falling sphere experiments with melts containing 2.3 and 5.6 wt.% H2O were carried out in an internally heated gas pressure vessel (IHPV) at 500 MPa confining pressure. The sinking velocity of Pt and Pd spheres and in one case of a corundum sphere was used to measure the melt viscosity. In addition, a creep experiment was performed at ambient pressure using a glass containing 2.73 wt.% H2O . A more water-rich glass (5.6 wt.% H2O ) was investigated with a high pressure parallel-plate viscometer at 400 MPa confining pressure in an IPHV. By combining our new data with previous results for a similar melt composition we derived the following expression to describe the viscosity η (in Pa s) as a function of temperature T (in K) and water content w (in wt.%)
82.
通过对重庆地区1999-2008年闪电定位系统监测地闪资料进行数理统计,重点对采用IEEE和DL/T620提供的公式获取的雷击建筑物绕击率进行对比分析,并对重庆全市进行雷击建筑物绕击率区划.结果表明:雷击建筑物绕击率随着滚球半径增大而增加;对于相同滚球半径,IEEE方法获取的雷击建筑物绕击率略高于实际,而低于GB/T21714提供的绕击率;在滚球半径小于120 m时,IEEE方法得到绕击率明显低于DL/T620方法,反之则高于DL/T620方法;采用IEEE公式获取的雷击建筑物绕击率与实际较为吻合,在此基础上获得了能客观反映重庆地区雷击建筑物绕击率表达式,并对不同防雷类别建筑物雷击绕击率进行了区划,为雷电灾害风险评估和防雷设计提供了可靠理论依据. 相似文献
83.
总强度磁异常各阶垂向导数换算新方法 总被引：2，自引：0，他引：2
磁异常垂直导数换算在磁性目标解释推断过程中具有重要意义。分析了总强度磁异常各阶垂向导数频率转换因子的滤波特性,指出常规傅立叶变换法在求解总强度磁异常各阶垂向导数时,观测数据中高频噪声会显著放大,甚至会淹没掉真实信息。从理论上证明了总强度磁异常沿垂直方向的积分和各阶导数均为调和函数,在此基础上,提出联合采用空间域和频率域运算求解其沿垂直方向的各阶导数。该方法的基本思路是：利用频率域转换关系,计算平面上总强度磁异常沿垂直方向的积分值;选择三点二阶中心差分或双三次样条曲线函数法计算总强度磁异常垂向积分值沿水平方向的二阶导数;最后将二阶水平导数代入拉普拉斯方程求解出总强度磁异常的垂向一阶导数;以总强度磁异常及其垂向一阶导数沿水平方向的二阶导数为基础,结合拉普拉斯方程,可进一步求解出总强度磁异常任意阶垂向导数。同时,为了研究提出方法的有效性,采用球体磁场模型进行验证,并首次推导了地磁场方向和磁化强度方向不一致时,球体总强度磁异常沿垂直方向的一阶和二阶导数表达式。经研究表明：提出的方法换算得到的垂向导数结果精度明显优于常规傅立叶变换法换算结果,且具有较强的抗噪能力,尤其是在计算高阶导数时效果更加明显。 相似文献
84.
提出了一种基于空间微分块与动态球判定策略的k近邻快速搜索算法。该算法以空间包围盒为基础,首先对空间进行微分块,将离散点分配到子空间;然后,以计算点为球心建立动态球,确定k近邻候选点。球半径可根据空间包围盒的大小、离散点数量和k近邻点数进行估算和优化。实验结果表明,该算法可快速完成k近邻搜索,运行稳定可靠。 相似文献
85.
A Comparative Study of Methods for Delineating Sphere of Urban Influence: A Case Study on Central China 总被引：1，自引：1，他引：0
A number of urban and regional plans have been developed with the advancement of urbanization and regional integration, among which the delineation of sphere of urban influence and improvement of integration between the city and its hinterland have be- come vital important for guiding practices. In terms of delineating sphere of urban influence, existing studies have been focused on static study by using single year data or single method, resulting in a lack of time-series longitudinal analysis or comprehensive analysis based on multiple methods This study emphasizes on comparing two methods from both the theoretical and empirical perspective. Both gravity model and improwd field model are applied to the selected study area for measurements and comparison, to explore their strengths and weaknesses. A research framework for comprehensive analysis on delineating sphere of urban influence is proposed. In the end, the differences of deli：aeating methods are illustrated and the feasibility of comprehensive analysis is discussed. Recommendations are provided for selecting appropriate methods for delineating sphere of urban influence or developing regional hierarchy system plans and urban spatial structure schemes. 相似文献
86.
Abstract This paper presents the first attempt to examine the stability of a poloidal magnetic field in a rapidly rotating spherical shell of electrically conducting fluid. We find that a steady axisymmetric poloidal magnetic field loses its stability to a non-axisymmetric perturbation when the Elsasser number A based on the maximum strength of the field exceeds a value about 20. Comparing this with observed fields, we find that, for any reasonable estimates of the appropriate parameters in planetary interiors, our theory predicts that all planetary poloidal fields are stable, with the possible exception of Jupiter. The present study therefore provides strong support for the physical relevance of magnetic stability analysis to planetary dynamos. We find that the fluid motions driven by magnetic instabilities are characterized by a nearly two-dimensional columnar structure attempting to satisfy the Proudman-Taylor theorm. This suggests that the most rapidly growing perturbation arranges itself in such a way that the geostrophic condition is satisfied to leading order. A particularly interesting feature is that, for the most unstable mode, contours of the non-axisymmetric azimuthal flow are closely aligned with the basic axisymmetric poloidal magnetic field lines. As a result, the amplitude of the azimuthal component of the instability is smaller than or comparable with that of the poloidal component, in contrast with the instabilities generated by toroidal decay modes (Zhang and Fearn, 1994). It is shown, by examining the same system with and without fluid inertia, that fluid inertia plays a secondary role when the magnetic Taylor number Tm ? 105. We find that the direction of propagation of hydromagnetic waves driven by the instability is influenced strongly by the size of the inner core. 相似文献
87.
以白家疃地震台为实验点,于2008年3月21日完成对该台"九五"前兆仪器针对"十五"台网进行整合改造。通过为期13个月的运行结果可以看出,其改造方案成本低,技术可行,产出数据可靠,为"九五"前兆台站整体接入"十五"管理系统提供了低成本、高效可靠的技术参考。 相似文献
88.
海洋研究通用信息平台的开发是1个复杂的系统工程,其中订制流程的创建和执行,以及适用于海洋用户的可视化类库设计在整个软件体系结构中占有重要地位.结合海洋研究领域需求的特点,以面向对象设计模式为基础,研究并实现‘系列解决这些问题的框架.这些框架明确各层之间的纵向和横向关系,通过统一的抽象接口进行通信,降低层次之间的耦合度.实验表明,该框架的建立对提高软件重用度、增强系统的可扩展性和可维护性等都有重要意义. 相似文献
89.
Some traditional methods, such as the velocity-azimuth display (VAD) and the velocity-azimuth processing (VAP), have been widely usedto retrieve the 3-D wind field from single-Doppler radar data because of their relative conceptual and practical simplicity. The advantage of VAD is that it is not affected by small-scale perturbations of the radial wind along the azimuth, to which the VAP method is very sensitive. Nevertheless, the spatial resolution of the VAD method is very poor
compared to the VAP method.
We show, in this study, that these two retrieval methods are actually related with each other and they are two special applications of a retrieval function based on the azimuthal uniform-wind assumption for a given azimuthal interval [θ1, θ2]. When using this retrieval function to retrieve wind fields, the azimuthal interval used in retrieval can be adjusted according to the requirement of smoothness or resolution. The larger (smaller) the azimuthal interval is, the coarser (finer) the horizontal resolution of retrieved wind field is, and the more insensitive (sensitive) the retrieval method is to small-scale perturbations. Because the full information within the azimuthal interval [θ1, θ2],instead of the information at two terminal points only, i.e., azimuths θ1 and θ2, is used to retrieve the wind fields, this method is referred to as the integrating VAP (IVAP) method, wherein the horizontal wind field is retrieved by using the Doppler velocity over the part of circumference, delimited by the given azimuthal interval times the scan radius. By contrast,the VAP method uses only the velocities at two terminal points of the given azimuthal interval. Therefore, the IVAP method has a filtering function, and the filtering rate can be controlled by adjusting the azimuthal interval. The filter such as that used in the pre-processing of the VAP method is no longer necessary for the IVAP method. When the retrieval azimuthal interval is as large as a whole circumference, the IVAP becomes the VAD. On the other hand, if only two neighboring azimuthal data are used, the IVAP becomes the VAP.
The frequency response function of IVAP indicates that the IVAP method can filter out shortwaves, and a larger azimuthal interval leads to stronger filtering ability, therefore a smoother retrieved wind field.
The shortwave filter function of the IVAP method is tested by an ideal experiment wherein the radar observations are artificially created by a uniform flow superposed with random disturbances. The VAP and IVAP methods are used in wind retrieval, respectively, and give different results for different azimuthal intervals (i.e., 6°, 12°, 24°, and 48°). Because the VAP method is sensitive to small disturbances, the retrieved winds have larger errors for all different azimuthal intervals. However, the retrieved wind by the IVAP method has smaller errors when the azimuthal interval is larger due to its shortwave filter function.
An experiment for an idealized linear wind field is also carried out to demonstrate the effect of the retrieval azimuthal interval on the IVAP method. The results show that a short interval gives the retrieval close to the “true" wind field with a linear distribution. When increasing the interval, the retrieval is smoothed and can represent only the mean wind field. 相似文献
90.