智能结构及其控制系统集成优化设计

将智能结构的振动控制性能指标和集成结构的质量为目标函数，结构尺寸参数和控制系统的控制参数同时作为独立的设计变量，并施加约束条件，从而将智能结构及其控制系统集成优化设计问题转化为多目标数学规化问题，数值结果表明，利用本文方法设计出的智能结构及其控制系统，能极大地抑制系统的振动。     

红外型空空导弹智能制导律研究

本文论述了红外型空空导弹应用智能控制的理论基础及结构特点，以多级智能控制的框架和机理设计出以比例导引为主、智能控制为辅的变指令智能制导律，并编制计算机软件以数字仿真的形式验证变指令智能制导规律的有效性和可行性     

星载SAR模糊特性及其工程设计

分析了星载合成孔径雷达产生模糊的机理及其与系统参数的关系，叙述了在宽广可视观测带曲，达到较好图像模糊度特性的优化设计原则，并提出了星载ＳＡＲ模糊性能的工程设计方法。     

The Brazilian scientific microsatellite SACI-1

The National Space Research Institute (INPE) is developing the first Brazilian Scientific Microsatellite (SACI-1) based on the vanguard technology and on the experience acquired through projects developed by Brazilian Space Program. The SACI-1 is a 750km polar orbit satellite. The spacecraft will combine spin stabilization with geomagnetic control and has a total mass of 60 kg. The overall dimensions are 640×470×470 mm. The SACI-1 satellite shall be launched together with CBERS (China-Brazil Earth Resource Satellite). Its platform is being designed for multiple mission applications. The Brazilian Academy of Sciences has selected four scientific payloads that characterize the mission. The scientific experiments are: ORCAS (Solar and Anomalous Cosmic Rays Observation in the Magnetosphere), PLASMEX (Study of Plasma Bubbles), FOTSAT (Airglow Photometer), and MAGNEX (Geomagnetic Experiment).     

具L2有界不确定性扰动系统最优跟踪问题的时域解

本文对Ｌ２有界不确定性扰动下的一性系统在时域提出Ｍａｘｍｉｎ最优跟踪问题，给出了问题的时域状态反馈解，这一问题与相应的Ｈ∞问题具有某种一致性，因此，问题的求解方法可为解决领域不确定系统的Ｈ∞最优跟踪问题提供一种时域途径。     

仿真模拟技术在固体火箭发动机操作训练中的应用

从导弹部队操作训练的角度出发,论述了固体火箭发动机仿真模拟训练的必要性和可行性,以及设想的仿真模拟训练系统的组成和功用.     

Drying as one of the extreme factors for the microflora of the atmosphere

An investigation of the effects of drying and drying-rewetting cycles under vacuum conditions of 10(-2) torr at -30 degrees C on conidia of the atmospheric strain Penicillium chrysogenum from 48-77 km heights, collected by meteorological rockets found that survival and restoration of the initial physiological properties were possible through some very efficient protective cellular mechanisms. Such adaptive possibilities explain the widespread diffusion of microbial cells throughout the biosphere of our planet.     

Phugoid oscillations in optimal reentry trajectories

A major problem with operations of lifting reentry vehicle having an aft center-of-gravity location due to large engine mass at the rear is the required hypersonic trim to fight the desired trajectory. This condition is most severe for lifting maneuvers. As a first step toward analyzing this problem, this paper considers the lift requirement for some basic maneuvers in the plane of a great circle. Considerations are given to optimal lift control for achieving the maximization of either the final altitude, speed or range. For the maximum-range problem, phugoid oscillation along an optimal trajectory is less severe as compared to a glide with maximum lift-to-drag ratio. An explicit formula for the number of oscillations for an entry from orbital speed is proposed.     

含碳酸钙的负压强指数复合固体推进剂燃烧机理

本文采用激光阴影高速摄影、扫描电子显微镜、X光电子能谱,对含和不含CaCO_(3)的三种夹心件及SO4-5A PU复合推进剂的燃烧过程、燃面形貌、化学成分和覆盖分数分别进行了研究和测定。结果表明:CaCO_(3)在低压下(〈1.96MPa)提高AP的燃速,在高压下(〉1.96MPa)起降速作用;CaCO_(3)与AP反应生成CaCl_2,并促使AP熔化;燃面上CaCl_2含量随压强上升而增加;PU熔化流动对AP表面的覆盖在mesa区内随压强而升高,在非mesa区的低压区也存在。基于以上实验结果,对含CaCO_(3)的PU负压强指数推进剂的燃烧机理进行了讨论。     

"Signal" search for intelligence in the galactic nucleus with the array of the Lowlands

In August, 1981, the Westerbork Synthesis Radio Telescope was used for 4 h to search for narrowband pulsing radio beacons in the direction of the Galactic Center. By using both the spatial discrimination and temporal stability available to an interferometric measurement, weak intermittent signals can be detected even in the face of the strong, naturally caused radiation from this region. A radio beacon within our bandwidth, centered on the 21 cm neutral hydrogen line, would be recognizable if it had a repetition period between 40 sec and 1/2 h. The rms sensitivity to point sources was approximately 50 mJy/cycle, and the detection limit was 500 mJy/cycle. The limit degrades for pulse widths < 0.02s. No repetitive signals were found. For a swept, narrow-band radio beacon constrained to the Galactic Disk (beamwidth = 0.02 rad), our detection limit corresponds to a transmitter power of 10(11) MW at the Galactic Center.