离散面目标毁伤概率算法和预报公式

本文描述了离散面目标毁伤概率的数学模型，利用均匀设计的方法安排仿真计算的数据，并给出了一个预报公式，可供导弹初步设计时使用。仿真结果表明，导弹射击精度CEP(平面)对毁伤概率的影响相对点目标而言要小，在设计针对离散面目标的飞航导弹时，对平面精度指标可以在一定程度上放松要求，提高末段高度控制精度，以提高全武器系统的作战效能。     

BTT导弹的最优导引规律

本文假定自动驾驶仪及弹体的动态特性为一阶环节,考虑了目标机动和导弹的姿态,用工作点线化方法,得到了以脱靶量和控制总能量为最小的二次型性能指标及以法向加速度和滚动角速度为控制变量的BTT导弹的最优导引规律。用简化模型进行了数值仿真计算,结果表明所推导的导引规律,可以拦截机动目标,具有良好的导引精度,有一定的工程实用价值。     

非连续增强镁基复合材料研究

采用液态浸渍法制备ＳｉＣ晶须和Ｂ４Ｃ颗粒混杂增强剂，成功地制备出增强剂含量为２４％的复合材料，并对材料的机械性能进行了测试，复合材料的抗拉强度达到了４１６ＭＰａ，弹性模量达到了８０ＧＰａ，较其基体材料分别提高了５３％和１１０％。对材料的断口分析表明，增强剂的均匀分布与晶须与基体之间的牢固结合，是复合材料具有较高机械性能的原因，而颗粒与基体界面间的开裂，以及基体共晶相的脆性开裂是复合材料塑性低的主要     

BTT导弹的H∞/加权混合灵敏度自动驾驶仪设计方法

本文用Ｈ∞／加权混合灵敏度方法设计某型地对空ＢＴＴ导弹的鲁棒自动驾驶仪。结果表明：基于标准弹道上某特征点的一个确定数学模型设计的Ｈ∞／加权混合灵敏度自动驾驶仪，可控制ＢＴＴ导弹沿标准弹道的全弹道稳定、准确地飞行，且能适应目标在一定飞行空域内的变化。     

月球探测器软着陆精确建模及最优轨道设计

针对探测器月面软着陆问题,在考虑月球自转的基础上建立了月球探测器在三维空间飞行的精确动力学模型。以燃耗最优为指标,利用Pontryagin极大值原理,得到了发动机推力开关曲线和推力方向角的最优控制律。综合考虑落点位置和速度约束求解两点边值问题,得到了探测器软着陆的最优轨线。仿真研究表明本文建立的精确动力学模型相对于不考虑月球自转的动力学模型可以有效提高探测器落点位置精度。     

Amino aciduria in weightlessness

Urinary excretion of amino acids by the 9 Skylab crewmen was studied as an indicator of the metabolic effects caused by exposure to the space flight environment. Intake was consistent in quality and quantity throughout the 28, 59 and 84-day flights for each of the crewmen and complete collections were accomplished. The results indicated an increased excretion in most amino acids during the first month of flight which remained elevated in the second and third months but to a lesser extent. Additional indications of change in muscle and skeletal metabolism were observed. These results point to the desirability of obtaining additional indices of alterations in protein synthetic processes in conjunction with future space flights.     

Energetic particle transport coefficients in the heliosphere

It is the purpose of this review to summarize and discuss recent research done in the field of particle propagation in the heliosphere. Several lines of approach have been followed to treat this problem. As a starting point the different forms of the transport equation are discussed. Quasi-Linear Theory (QLT) relates the power contained in fluctuations of the Interplanetary Magnetic Field (IMF) to the transport coefficients of energetic particles, an outline of the basic results of this theory is presented followed by a discussion of subsequent corrections made to the original formulation with an emphasis in recent developments where the effects of wave polarization, its propagation respect to the solar wind and the dissipation of power at large frequencies have been taken into account. The numerical approach using test particle trajectory integrations to obtain transport coefficients based on in situ satellite measureents is also discussed. It is well known that the determination of the particles mean free path for solar particle events by alternative methods leads to conflicting results, corrections made to original QLT are attempts to bridge the gap. Determination of the transport parameters from different lines of approach in a comparative basis have been done recently by calculating power spectra of IMF measured at the time solar particles were detected on the same spaceprobe, and performing numerical simulations with equivalent IMF data. Some of the results of such studies point to the solution of the conflicting determinations of the mean free path which has existed for nearly 30 years. An assesment of the present situation in this respect is given. Numerical determinations of transport parameters in the outer heliosphere are also reviewed and its consequences for solar modulation of galactic cosmic rays discussed. Space Science Reviews 62: Printed in Belgium.     

参数空间中鲁棒镇定问题

研究了线性定常控制系统(SIMO或MISO)在结构参数扰动下的鲁棒稳定性。对于固定控制器,如果在标称参数p~0下闭环渐稳,我们指出了在参数空间中找出比中心位于p_0的最大稳定超球还要大的稳定超球的构造方法,可以求出包含p_0的一个最大的稳定超球,从而得到更大的稳定锥形域。改善了鲁棒稳定性判据,得到了一个同时镇定系统族的充分条件。     

实时仿真中的数据重构与误差分析

动态系统实时仿真中的数据重构现象，以及数据重构所产生的动态误差在本文中作了分析和讨论。实例说明了补偿这种误差的方法。