机载箔条弹最佳使用时机仿真研究

为了寻求箔条弹的最佳使用时机,通过建立箔条弹、飞机和导弹三者的数学模型,以弹机之间的最小距离为准则,在计算机仿真的基础上给出弹机之间最小距离和最佳使用时机与各种因素的关系,可以得到在不同的情况下的最佳投放时机;同时通过仿真模型的建立,得出一种寻求箔条弹最佳使用时机的新方法。     

在轨目标逼近远程导引律设计

利用最优多脉冲方法,对目标航天器逼近过程的远程导引段轨道进行设计.基于Lawden主矢量理论,解决固定时间、燃料最省的逼近轨道问题.通过仿真分析了固定初始条件时燃料消耗量随着转移时间的变化关系.对于燃料和时间均有约束的情况,给出了求解燃料最省和时间最小的多目标优化问题的方法.这一研究对于评估具体任务的燃料消耗和转移时间有重要意义.     

侧摆摄影偏流角和速高比的计算模型

像移会使图像质量退化,分辨率下降,为此必须对像移进行补偿。文章从空间相机像移补偿的角度出发,建立了卫星遥感中偏流角和速高比的概念;通过坐标转换推导出了卫星在星下点、侧摆、俯仰摄影模式下偏流角和速高比的计算公式,从而可考虑对所产生的像移进行补偿。     

五棱锥SGCMGs失效时奇异构型几何分析及操纵律设计

单框架控制力矩陀螺群(SGCMGs)的奇异构型几何分析及相应的操纵律设计是其在使用中遇到的主要问题。针对五棱锥SGCMGs构型及其单只失效后的奇异情况进行几何分析,考虑五棱锥构型单只SGCMG失效后显奇异点深入角动量体内部这一特性,设计了一种既能充分利用零空间运动,又能实现显奇异点规避的SGCMGs操纵律。仿真分析结果表明:设计改进后的操纵律能在有效解决五棱锥SGCMGs构型中单只陀螺失效后带来内部复杂奇异问题的同时,实现控制精度的大幅提升。     

基于GPS的地球资源卫星精密星历外推新方法

随着技术的发展,通过星载GPS接收机直接确定卫星星历成为卫星定位的一个重要手段.GPS接收机获取的卫星星历数据是某一时刻的瞬时状态,要获取连续的卫星星历数据还需要进一步处理.常用的处理方法有几何法与动力学法.在GPS接收机给定瞬时星历频率较低的情况下,几何法的计算误差比较大,特别是只有一组瞬时星历时,无法用几何法进行轨道的外推.在分析地球资源卫星轨道特点的基础上,提出一种新的轨道缩减动力模型,该模型将卫星运动在直角坐标系中分解为简谐运动,利用模型实现了轨道外推的算法.通过试验验证,该算法可以达到较高的精度.      

高超声速湍流分离激波运动和压力脉动

简述在Ｍ∞＝７．８、Ｒｅ∞＝３．５×１０７／ｍ气流条件下,无后掠和后掠压缩拐角及直立半圆柱前缘舵上游平板干扰区壁面压力脉动测量结果及其分离激波运动特性。     

双脉冲固体火箭发动机隔塞运动特性

以双脉冲固体火箭发动机隔塞的运动过程为研究对象,搭建了脉冲隔离装置冷气冲击实验平台,获得了隔塞在Ⅰ脉冲燃烧室中的运动规律.采用动态结构嵌套网格方法,对隔塞的运动过程进行了数值模拟,分析了隔塞运动过程中流场结构,揭示了隔塞运动规律的形成机制.研究结果表明:对于单孔隔板,隔塞在燃烧室中沿轴向平稳运动,随着驱动压强的上升,隔...     

一种基于航摄图像特性的H.263压缩算法的改进

研究了航摄视频图像的特性,并根据航摄视频图像的特性,从预测初始搜索点、搜索策略和半像素精度运动估值方面改进了H.263标准中的运动估计算法。实验结果表明,针对航摄图像特性改进的算法比全搜索算法和三步搜索算法具有更高的搜索效率。     

机床主轴径向回转误差的测试与研究

给出了一种主轴回转误差动态测量的误差分离方法,提出了一套主轴回转精度的动态测试系统。该系统由位移测试单元、采样时钟单元、数据采集卡、通用计算机及数据处理软件组成。     

In-flight testing of the injection of the LISA Pathfinder test mass into a geodesic

LISA Pathfinder is a technology demonstrator space mission, aimed at testing key technologies for detecting gravitational waves in space. The mission is the precursor of LISA, the first space gravitational waves observatory, whose launch is scheduled for 2034. The LISA Pathfinder scientific payload includes two gravitational reference sensors (GRSs), each one containing a test mass (TM), which is the sensing body of the experiment. A mission critical task is to set each TM into a pure geodesic motion, i.e. guaranteeing an extremely low acceleration noise in the sub-Hertz frequency bandwidth. The grabbing positioning and release mechanism (GPRM), responsible for the injection of the TM into a geodesic trajectory, was widely tested on ground, with the limitations imposed by the 1-g environment. The experiments showed that the mechanism, working in its nominal conditions, is capable of releasing the TM into free-fall fulfilling the very strict constraint imposed on the TM residual velocity, in order to allow its capture on behalf of the electrostatic actuation.However, the first in-flight releases produced unexpected residual velocity components, for both the TMs. Moreover, all the residual velocity components were greater than maximum value set by the requirements. The main suspect is that unexpected contacts took place between the TM and the surroundings bodies. As a consequence, ad hoc manual release procedures had to be adopted for the few following injections performed during the nominal mission. These procedures still resulted in non compliant TM states which were captured only after impacts. However, such procedures seem not practicable for LISA, both for the limited repeatability of the system and for the unmanageable time lag of the telemetry/telecommand signals (about 4400 s). For this reason, at the end of the mission, the GPRM was deeply tested in-flight, performing a large number of releases, according to different strategies. The tests were carried out in order to understand the unexpected dynamics and limit its effects on the final injection. Some risk mitigation maneuvers have been tested aimed at minimizing the vibration of the system at the release and improving the alignment between the mechanism and the TM. However, no overall optimal release strategy to be implemented in LISA could be found, because the two GPRMs behaved differently.