并行编码选择扩频通信方式

提出了并行编码选择扩频通信方式，给出了并行编码选择扩频通信方式的系统模型，分析其通信性能。讨论了系统的误差概率和系统的信息数据传输能力，给出了数学模型和计算公式。结果表明，该系统与其它几种扩频通信方式相比较具有最高的信息传输效率。但其可靠性稍差，这说明通信的有效性的提高是以降低可靠性为代价的。本方式适合于传输信道具有较高信噪比的情况下使用。     

雷达本振相位噪声的数字仿真技术

在现代雷达和通讯系统中 ,本振相位噪声越来越成为决定系统性能的关键因素。分析了本振调相、调幅噪声对相参雷达系统探测性能的影响 ,给出了主杂波环境下雷达发射机调相噪声以及发射机泄漏的调幅噪声的数字仿真模型。在雷达数字仿真系统中使用这些模型 ,可以在各种环境下定量分析微波本振相位噪声对目标探测性能的影响 ,对昂贵的微波系统提出满足总体设计要求的合理指标。     

凝聚相粒子在喷管喉部沉积规律的理论预示

以金属粉末为添加剂的固体燃料,在燃烧后金属氧化物以凝聚态的形式在喷管中流动。对于工作时间长、喷喉较小的固体火箭发动机,凝相粒子在喷管喉部的沉积严重地影响到发动机的内弹道性能,甚至引起发动机的爆破事故。因此,搞清沉积规律是十分必要的。 本文根据凝相粒子的运动规律以及关于沉积层的移动边界传热问题的分析,提供了一个关于沉积速度的理论预估方法。通过算例,证明理论预估与实验资料是十分吻合的。     

含硼推进剂燃烧性能的改善

综述了改善含硼推进剂燃烧性能的研究状况，包括硼粒子表面包覆，火箭冲压发动机设计的改进，添加新的组分，调整配方以及改进推进剂制造工艺等，这些措施都可以提高含硼推进剂的燃烧性能。     

柔性梁结构的时滞主动控制

对考虑时滞影响的柔性悬臂梁的离散最优控制进行了研究。首先采用独立模态空间方法给出包含有时滞项的控制模态方程，然后将之离散化并通过状态变量增广转化成不含时滞的标准离散形式。离散形式的性能指标也转化成增广形式。则离散时滞最优控制律可以针对增广的系统进行设计。因在最初的系统动力方程中就考虑了时滞项，且在推导离散模态控制律的过程中无近似处理，因而所给控制方法易于保证控制系统的稳定性。另外，文中还给出了从实际测量中提取模态坐标和将模态控制力转换成实际控制力的方法。最后通过数值仿真对本文所提控制方法的可行性和效果进行了验证。仿真结果显示，采用本文所提控制方法能够有效地抑制结构的振动。若在控制设计中忽略时滞，有可能引起动力失稳。     

较小功率脉冲YAG激光填丝焊接技术的研究

介绍了利用较小功率脉冲YAG激光做热导焊接的激光填丝焊接技术;并讨论了微型结构件的激光 填丝焊接方法;给出了利用脉冲YAG激光做微型结构件的激光填丝焊接的较佳焊接工艺。     

On the free-vibration of rotating composite beams using a higher-order shear formulation

The free vibration behavior of rotating blades modeled as laminated composite, hollow (single celled) boxed beams is investigated. To this end, geometrically nonlinear structural model incorporating a number of non- classical effects such as anisotropy, heterogeneity, transverse shear flexibility, and warping inhibition is developed. Centrifugal and Coriolis force field effects are also considered in the formulation. However, Coriolis effect is discarded during the solution process. It is assumed that in-plane cross-sectional distortion is negligible. In contrast to the existing structural blade models, the traction free boundary conditions on the external surfaces of the beam are identically satisfied. The linearized dynamical equations and numerical results addressing the problem of the free vibration are supplied. Results obtained for the present higher-order shearable model are compared with those of the existing first-order shearable and the non-shearable structural models. Tailoring studies using the present model reveal an enhancement of eigenfrequency characteristics.     

光抽运小铯束频率标准中光频移的测量

对光抽运小铯束管的光频移进行了测量 ,并对结果进行了简要的分析 ,估算了射入Ramsey腔的相应光强。导致光频移的光源是抽运光和检测光通过漫反射进入微波腔的部分和原子束中的铯原子自发辐射所产生的荧光。     

Evolution of an electron beam pulse influenced by coulomb collision effects in the solar corona

Electrons accelerated in the corona during solar activity give rise to radio emission events that can be observed over a wide range of frequencies. Among different finer-scale structures in the dynamic spectra observed in the radio range, fast transients with extents of some milliseconds known as solar radio spikes are observed accompaning the background continuum emission. Fundamental to the generation of radio spikes is a propagating electron beam and following its evolution allows us to understand the physical processes occurring in the solar corona. With the use of a numerical Fokker–Planck code we follow a previous numerical study to simulate the propagation of an electron beam pulse injected in a small region at the top of a magnetic field and outwards the solar corona under typical flare conditions. It was found that in large ambient densities of ${10}^{10}$ cm⁻³ at the injection point, Coulomb collision effects have an important effect on the propagation of the electrons, causing that the injected electrons thermalize faster in a time of $0.1$ and $0.4$ s for an electron distribution with a low-energy cut off of 16 and 7 keV respectively and a spectral index of 3. For a tenous ambient medium of density ${10}^9$ cm⁻³ thermalization occurs only for an electron distribution with smaller low-energy cut off (7 keV) with a duration of $\approx$1.5 s, while for a larger low-energy cut off (16 keV) the loss of accelerated electrons is very slow, regardles of the spectral index ($3,7$). The electron loss time by Coulomb collisions, which depends on the low boundary ambient density, might be an important parameter that influences the generation of radio spikes due to the formation of instabilities in the corona.