The fundamental parameters of the central stars of eight WR ring nebulae

We describe work that has recently been completed on deriving the fundamental parameters of eight WR stars through the photoionization modelling of their surrounding nebulae using non-LTE WR flux distributions. The resulting effective temperatures range from 57 000–71 000 K for the WN4-5 stars and <30 000–42 000 K for the WN6-8 stars. The derived stellar parameters are compared with those obtained from stellar emission line modelling. We find good agreement for the hot early WN stars, indicating that the non-LTE WR flux distributions have essentially the correct shape in the crucial far-UV region. We find lower temperatures for the four cooler late WN stars, particularly for the two WN6 stars. For the nebulae surrounding these stars, we find that the model flux distributions produce too much nebular ionization. We suggest that these discrepancies arise because of the lack of line-blanketing in the WR atmospheres. For the WO1 central star of G2.4+1.4, with strong nebular He II 4686 A emission, we derive a temperature of 105 000 K, somewhat less than previous estimates. The positions of our eight WR stars on the H-R diagram are compared with the evolutionary tracks of Maeder (1990) for solar metallicity. In common with previous workers, we find that our derived luminosities are too low, giving an initial mass range of 25–40 M, below that expected for the majority of WR stars.     

Energetic particles at high latitudes

We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path _r which is approximately constant as a function of distancer. When particle propagation in three dimensions in the heliosphere is considered it is not sufficient to consider _r only. Jovian electrons can be used as probes to determine the parameters of three-dimensional diffusion. In the polar regions diffusion is dominated by its parallel component. Some predictions how should vary with latitude are discussed. For different choices of this variation we present expectations for intensity-time profiles of solar particle events during the Ulysses polar passages.     

结构/直角切割网格下时域有限体积法在计算电磁中的应用研究

 采用有限体积法直接求解时域麦克斯韦方程组，研究了二维圆柱、翼型和三维球体、立方体、双球体等典型完全导电目标的电磁散射问题。空间离散使用近似黎曼解构建网格通量，并针对二维结构网格、三维自适应直角切割网格分别给出重构方法，时间方向采用二步龙格库塔法。计算与理论、实验或文献结果符合良好。     

航空交流电机的电磁噪声分析

研究了航空电机定子径向振动模数，分析了电磁力波产生的原因，给出了径向电磁力波引起的振动及噪声的阶次，其值可由谐波磁场谱表求出。结合实例，分析了航空电机定转子激振力波阶次及电磁噪声的频率范围。     

流线追踪Busemann进气道设计参数的选择

为了研究型面设计马赫数、唇口偏移量对流线追踪Busemann进气道设计点性能的影响规律,寻求最佳性能的进气道,对设计马赫数为6,具有不同型面设计马赫数和唇口偏移量的流线追踪进气道进行了数值模拟。研究表明:选取低于马赫数6的型面设计马赫数,可获得较高的流量系数和增压比,而其压缩效率并不低;进气道唇口偏移量增大,会导致流量系数、增压比变小,但却有利于减小进气道内的分离程度,还会影响隔离段内的流动,因此唇口偏移量的选取需要综合考虑。     

飞行器动态稳定性参数的数值计算方法

本文提出了一种确定飞行器动态稳定性参数的数值方法。本文首先研究了气动力与飞行器运动状态参数之间的关系，在此基础上给出了稳定性参数的定义。根据这一定义并结合计算流力学和参数辨识方法，构造了计算飞行器稳定性参数的完整数值方法，数值实验表明，该方法具有通用性强和准确度较高的优点。     

火焰稳定器射流喷口形状对燃烧性能的影响

为了探讨层缘吹气式火焰稳定器的射流喷口形状对燃烧性能的影响，在来流50m/s，573K条件下，分别对连续长缝、不连续宽缝、均布圆孔三种不同喷口形状的火焰稳定器的燃烧性能进行了实验研究，对比了它们的贫熄特性、燃烧效率和流阻损失。研究发现，在实验条件范围内，连续长缝形喷口稳定器的燃烧性能较其他两种不连续喷口稳定器优越，具有较高的燃烧效率、较宽的贫熄边界和较小的流阻损失。     

蛇形进气道的电磁散射特性

 对一种进口与机身保形设计的蛇形进气道在Ku波段选择入射频率15 GHz情况下进行了电磁散射特性的实验和仿真研究，取得了蛇形进气道雷达散射截面(RCS)随方位角、迎角和终端的变化规律。研究结果表明: (1)该蛇形进气道在水平极化终端为风扇时±60° RCS均值为-24.33 dB·m²，垂直极化为-19.15 dB·m²，是一种低RCS进气道；(2)运用时域有限差分法计算所得的RCS随方位角变化曲线与实验曲线趋势基本一致，±60°均值误差在4 dB以内；(3)从进气道对称面电场(Ex)分布图可以看出入射波射入进气道并在内壁面产生多次反射，从而验证了蛇形进气道的设计思想并为在内通道关键反射点涂敷吸波材料实现蛇形进气道的高隐身提供了一个可行的研究平台。     

运输机总体参数和性能统计分析

 按照飞机设计的基本原理,通过对现有运输机总体参数和性能数据的统计分析,寻找现代运输机各个总体性能和性能参数之间存在的定量关系,得到了 1 6个经验公式和一些参数取值范围,为运输机概念设计提供了一些可用的数据。     

确定威布尔分布三参数的相关系数优化法

 根据本文给出的确定威布尔分布三参数的相关系数优化法求得的威布尔三参数,能使试验数据在威布尔概率坐标纸上最大限度地呈现为线性关系。