多飞行器测控技术的研究

提出了一种基于DBF和DMF-CDMA技术的多飞行器测控系统。首先描述了系统的工作原理，然后对DBF给出了全面和详细的计算机仿真，包括圆面阵DBF阵因子方向图仿真和DBF对多飞行器的搜索与跟踪仿真。最后对DMF-CDMA给出了实验结果。实验的硬软件巳达到实用水平。这些说明本文提出的多飞行器测控方案是可行的。     

固体火箭发动机试验模态分析技术研究

将固体火箭发动机划分为144个自由度，采用锤击法，单点激励多点响应（SIMO）对其在4种工况下进行了频率响应的测量，应用了多种方法进行模态参数识别和数据拟合，并对其结果进行比较，获得了发动机在各工况1kHz以内的各阶固有频率、振型和阻尼，并对试验模态分析技术在固体火箭发动机试验中的应用进行了研究。     

板料成形的数值分析及程序系统

本文讨论了板料成形的数值分析方法,并介绍一个能在微机上运行的程序系统——CASF(Computer Aided Sheetmetal Forming)01系统。 CASF01系统采用参数三次样条描述板金零件的几何外形,按弹-塑性流动理论用完全拉格朗日有限元法计算成形过程中的应力应变分布。由于参数样条的插值性和分段描述特点与有限元法的结构离散在基本思想和处理方法上的相似性,系统内曲面描述和力学分析程序间数据传递迅速方便。圆板胀形及其汽车零件的计算实例表明了CASF01系统的可靠性和实用性。     

异型封闭腔辐射几何学问题

讨论了解决异型封闭腔辐射几何学问题的几种方法:异型封闭腔内,表面间可见性的判断方法;优化异型封闭腔角系数计算的方法;确定异型封闭腔内定向辐射的壁面辐射源的方法.计算了两种结构喷管封闭腔内的角系数,并从角系数的互换性和完整性定理验证了方法的正确性和有效性,为异型封闭腔的辐射计算解决了几何问题.     

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.     

三通管复合胀形过程模拟

建立了三通管复合胀形的三维弹塑性有限元模型,研究了三通管液压复合胀形中,反压大小、加载路径以及加载时间等对胀形成形的影响。     

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。     

因康镍718合金的超塑成形和扩散连接

介绍了用于制造火箭发动机零件的因康镍７１８合金的超塑成形和扩散连接工艺。经特殊加工的细晶粒因康镍７１８合金具有促进的超塑性，历而能用于超塑成形相当复的零件。     

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。