自动氩弧焊控制电路的改进

为了对某航天产品的焊接焊缝的熔深控制在规定的范围内，对自动氩弧焊焊接设备的控制器作了改进，并设计了一套控制电路。实际应用证明，改进后的设备可靠性高，稳定性好，并可用于非接触引弧的各类直流焊机上。     

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。     

钛合金焊接件疲劳特性评估的当量Kt法

针对先进飞机结构广泛采用的钛合金焊接结构,提出了描述焊接件疲劳特性的当量理论应力集中系数Kt(K_te)的概念;建立了以钛合金材料疲劳性能为基础,通过一组谱载下钛合金焊接件疲劳试验来确定K_te的技术途径.以TC4钛合金氧弧焊试件为例给出了确定K_te的具体方法和结果.     

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.     

多层钎焊结构件超声C扫描信号特征分析

对多层钎焊件内层焊缝检测中产生的多重声束路径叠加现象进行了详细分析,并用计算机模拟超声检测中的叠加信号,总结出对等厚薄板钎焊缝阵结构内层焊缝的检测方法及C扫描时信号门放置的合理位置,并且在实际检测中验证了该方法的正确性.     

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。     

扩散焊接及其在航空航天领域的应用

扩散焊接是制造航空航天构件非常重要的连接技术。本文简略地介绍了它人特点，分类，连接机理，焊接设备以及它们在航空航天领域的应用。     

Ti3Al—Nb基合金的焊接性研究进展

介绍了Ti3Al-Nb基金属间化合物合金焊接性的研究状况，重点评述了其物理和焊接冶金特点、主要焊接工艺下的焊接性和焊后热处理对接头显微组织和力学性能的影响，指出了需深入研究的问题。