旋翼三维非定常跨音速绕流的数值模拟

 利用小扰动位势方程，用有限差分方法求解了旋翼跨音速流场。导出了严格的三维非定常位势方程远场无反射边界条件，并成功地用于数值计算中，缩小了物理求解域的空间尺度。采用了贴体坐标和网格加密技术，以得到合理的非均匀网格分布。应用较少的网格点数成功地计算了无升力情况下旋翼的三维非定常亚、跨音速绕流流场，得到了与实验结果符合良好的数值解     

跨声速粘性流中的翼型设计与分析

本文采用一种数值方法设计和分析跨声速翼型。几个算例表明,对于激波/边界层弱干扰和强干扰情形,该方法的结果与风洞实验值吻合良好。但是,当翼型表面出现分离时,两者的差别较大。     

高亚声速喷流近场的流-声关联

针对马赫数为0.9的圆口喷流,采用大涡模拟计算流场与声场,在与直接数值模拟(DNS)和实验数据比对验证的基础上,分析了中心线和剪切层湍流脉动信号与声信号的相关性,并进一步对中心线上温度信号进行相关性研究。结果表明:相关系数在中心线上势流核末端附近出现峰值,说明该处的湍流脉动信号对声压信号有重要贡献,而这一区域的流动的间歇性与对流速度均较高。同时,声压与中心线上的温度脉动和温度梯度径向分量的脉动也有较高相关性,但与温度梯度轴向分量的脉动相关性较低,表明在模拟的温度比下轴向温度梯度对近场声压贡献较小。     

Evaluation of uncertainty in gravity wave potential energy calculations through GPS radio occultation measurements

The application of the Global Positioning System (GPS) radio occultation (RO) method to the atmosphere enables the determination of height profiles of temperature, among other variables. From these measurements, gravity wave activity is usually quantified by calculating the potential energy through the integration of the ratio of perturbation and background temperatures between two given altitudes in each profile. The uncertainty in the estimation of wave activity depends on the systematic biases and random errors of the measured temperature, but also on additional factors like the selected vertical integration layer and the separation method between background and perturbation temperatures. In this study, the contributions of different parameters and variables to the uncertainty in the calculation of gravity wave potential energy in the lower stratosphere are investigated and quantified. In particular, a Monte Carlo method is used to evaluate the uncertainty that results from different GPS RO temperature error distributions. In addition, our analysis shows that RO data above 30 km height becomes dubious for gravity waves potential energy calculations.     

SuperDARN cross polar cap potential dependence on the solar wind conditions and comparisons with models

In this study SuperDARN Cross Polar Cap Potentials (CPCPs), collected over the year 2000, are investigated with a goal to statistically assess its relationship with various parameters of the solar wind and Interplanetary Magnetic Field (IMF). We show that SuperDARN CPCPs tend to cluster around discrete values, prescribed by the statistical model, unless the amount of points on each convection map is above ∼300. By selecting CPCP data obtained with radar coverage of >300 points, we investigate the CPCP relationship with IMF B_z and B_y, IMF clock angle, solar wind speed and dynamic pressure, Alfven velocity, Alfven–Mach number, and interplanetary electric field. Some reported tendencies, such as dependence upon IMF B_z, were found to be consistent with measurements by other instruments. We demonstrate that SuperDARN CPCPs show consistency with several theories/empirical models (predicting the CPCP) in terms of a linear trend but, on average, the slopes of the dependencies are at least two times smaller. We also determine the coupling function, out of those published in literature, best correlating with SuperDARN CPCPs.     

n维简并理想费米气体的化学势和热容量

本文对能谱为ε＝ａｐ＾ｓ的ｎ维并理想费米气体作了统一讨论，给出了它的一级近似遇米能，有限浊度下的化学势、内能以及热容量的表达式。     

环形磁铁空间磁场的解析计算与仿真

从永磁体的磁荷模型出发,运用标量磁位法、广义二项式定理、矢量叠加原理等建立了环形磁铁在磁体外部空间磁场分布的解析表达式,并在MATLAB仿真软件中进行了计算。利用三维数字式特斯拉计实际测量了两种规格的永磁体的磁场分布,利用Ansoft Maxwell电磁场分析软件建立了两种永磁体在磁体外部空间的磁场分布,通过对比解析计算结果、实际测量结果和Ansoft Maxwell仿真结果发现解析表达式很好地反映了永磁环空间磁场的分布规律,误差不超过7％,从而验证了解析表达式的正确性。     

基于通用航空的空中交通管制压力和风险评估方法的探讨

飞行流量管理现已成为业内人士经常研究和谈论的话题,也是民航发展过程中必须解决的重要问题。与运输航空不同,通用航空的流量管理和评估问题却少有人问津。本文结合国内最大的通用航空基地——民航飞行学院的实际运行情况,把空中交通管制工作风险按照能量的概念数据化,借鉴能量控制的理论,提出风险势能的概念,并对这一概念在通用航空空中交通流量管理中的应用进行了探讨。     

跨声速非匀熵全速位方程的有限元数值解(英文)

本文改进了传统全速位方程的有限元数值解,既保留了全速位方程简单的优点又考虑了出现激波后流场不是匀熵的特点,对密度和后缘库塔条件进行修正,改善了计算结果。文中给出翼型和机翼的算例,其结果与传统全速位方程的结果相比,激波的位置偏往上游,强度较弱,这个趋势使结果较接近于欧拉方程的解。     

一种热电势的简易表达法

当具有不同温度分布的多种导体连接在一个环路中时,按照帕尔贴电势和汤姆逊电势分析环路中的总的热电势是困难的。选择一些导体作为标准电极,就能把总的热电势分成一系列单一导体的独立热电势,用这个方法,分析工作将变得十分简单。