大型复合材料结构优化设计方法研究

建立了适合于大型复合材料结构的优化设计方法，该方法在复合材料结构有限元分析的基础上对复合材料结构进行优化设计。在建立有限元模型时应用了区域划分技术，然后对结构分两级进行优化：第一级是对结构的铺层角度进行优化。第二级对结构的铺层厚度进行优化。最后，以工字梁结构为例，进行了算法验证。     

战术固体火箭发动机按费用优化设计

论述了按费用设计的概念和方法，在５种战术固体火箭发动机制造成本数据统计分析的基础上，以部件重量作为模型参数，建立了适合于战术固体发动机的喷管，装药和壳体成本模型，根据这些成本模型，对某地－空战术导弹火箭发动机以冲费和为目标函数进行按费用优化设计，所得结果通过与实际发动机试车结果及制造成本比较，表明以作为参数的成本模型合理，按费用优化设计技术可行，经济上合理。     

基于遗传算法和空间推进方法的高超声速进气道优化设计研究

将遗传算法（单目标遗传算法GA和多目标遗传算法NSGA-Ⅱ、NCGA）与高效、高精度的卒间推进方法——SSPNS（Single-sweep Parabolized Navier-Stokes Algorithm）流场计算方法相结合，对二维高超声速进气道进行了气动优化设计研究。在单目标优化设计中以巡航点（Ma=7．0）的总压恢复最大为设计目标，多目标设计中则在巡航点分别考察了总压恢复最大-压升最大两目标模型、总压恢复最大-压升最大-阻力系数最小三目标模型。优化设计结果表明，单目标设计使得总压恢复有明显提高；多目标优化设计所得的Pareto最优前沿为设计者提供了可靠的设计依据。为了兼顾巡航点和加速爬升段的综合忭能，采用多目标优化方法对进气道进行了多点优化设计，并开展了基于等动压弹道的设计点选择问题初步研究。计算结果表明，若将设计点选在Ma=6．5左右，则进气道的综合性能较好。     

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。     

Estimation of sea surface temperature, wind speed and water vapor with microwave radiometer data based on simulated annealing

A method for estimation of sea surface temperature, ocean wind speed and water vapor with microwave radiometer data based on simulated annealing is proposed. The proposed method shows about 60% improvement of sea surface temperature estimation accuracy in comparison to the existing method using Newton’s iterative algorithm.     

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.     

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。